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Author name code: vandessel
ADS astronomy entries on 2022-09-14
author:Van Dessel, Edwin L.J.

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Title: Mesures d'Étoiles doubles visuelles obtenues - l'observatoire
    de nice en 1968 (lunette de 50 cm) et avec la lunette Équatoriale
de 45 cm de l'observatoire royal de belgique de 1969 - 1974 Title:
    Mesures d'Étoiles doubles visuelles obtenues - l'observatoire de
    nice en 1968 (lunette de 50 cm) et avec la lunette Équatoriale
de 45 cm de l'observatoire royal de belgique de 1969 - 1974 Title:
    Measurements of visual double stars collected with the 50-cm refractor
    of the observatoire denice in1968 and with the45-cm refractor of
    theobservatoire royal de belgique from 1969 to 1974.
Authors: Lampens, P.; Van Dessel, E.; Rabtach, S.; Durand, P.
2011O&T....79...17L    Altcode:
  We present in an electronic form the measurements of the relative
  positions of 129 visual double and multiple systems performed by Dr
  E. Van Dessel during the years 1968-1974. In the summer of 1968, 64
  measurements of 38 different systems were collected at the Observatoire
  de Nice. From 1969 till 1974, 295 measurements of 91 systems were
  collected at the Observatoire royal de Belgique. The original booklet of
  the observations was put at our disposal for this task performed by one
  of us (S.R.). In addition, we also present the residuals in the sense
  (Observed-Calculated) based on the orbits listed in the Sixth Catalog
  of Orbits of Visual Double Stars (Hartkopf and Mason, 2012). <P />2

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Title: Division i / Commission 8 / Working Group Astrographic
    Catalogue and Carte du Ciel Plates
Authors: Bucciarelli, Beatrice; Fresnau, Alain; Abad, Carlos; Argyle,
   Robert W.; Biggs, James; Brosch, Noah; Coyne, George V.; Davoust,
   Emmanuael; De Cuyper, Jean-Pierre M.; van Dessel, Edwin L.; Ducourant,
   Christine; Fierro, Ivan H. Bustos; Geffert, Michael; Glushkova, Elena
   V.; Irwin, Michael J.; Jones, Dayton L.; Lumme, Kari A.; Muiños,
   J. L.; Odenkirchen, Michael; Orellana, Rosa B.; Pauwels, Thierry;
   Rafferty, Theodore J.; Sanchez, M.; Sanner, Jörg; Tsvetkov, Milcho
   K.; Vaughan, Alan E.
2007IAUTB..26...95B    Altcode:
  Various experiments have definitely demonstrated that one-micron
  accuracy (0.″06) on the definition of stellar images on CdC
  plates cannot be claimed, as it was speculated back in 1999. More
  realistically, a 2-3 micron accuracy is achievable, getting worse
  toward the survey magnitude limit, with an average magnitude error
  of 0.3. The level of astrometric accuracy corresponds to a 0.″2 -
  0.″3 error in position at Epoch 1900, which, once used as first
  Epoch for proper motion determination in combination with modern epoch
  observations, can produce errors at the level of 2-5 mas/yr, thereby
  allowing to detect stellar motions larger than 0.″01/yr, which at a
  distance of 500 pc from the Sun correspond to ~25-60 km/s tangential
  velocity. Therefore, the AC/CdC heritage collection can be regarded
  as a highly valuable first-epoch material, e.g., for the realization
  of a Tycho-2 extension to fainter magnitudes (~15 photographic),
  especially in selected areas where radial velocity data are available,
  for the exploration of stellar kinematics beyond our solar neighborhood.

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Title: VizieR Online Data Catalog: Photometric standards around
    gravitational lenses (Nakos+ 2003)
Authors: Nakos, T.; Ofek, E. O.; Boumis, P.; Cuypers, J.;
   Sinachopoulos, D.; van Dessel, E.; Gal-Yam, A.; Papamastorakis, J.
2003yCat..34021157N    Altcode:
  We present a catalog of secondary photometric standard stars in
  the neighborhood of 14 gravitationally lensed quasars. These stars
  were verified to be non variable using long-term monitoring. <P
  />The instrumental magnitudes of the new standard stars have been
  transformed to the Johnson-Cousins BV(RI)c photometric system. For ten
  gravitational lenses (GLs) we also provide the BV(RI)c mean magnitudes
  of the integrated flux of all the lens components, for the epochs of
  the photometric calibration. <P />(3 data files).

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Title: A catalog of secondary photometric standard stars around
    gravitational lenses
Authors: Nakos, Th.; Ofek, E. O.; Boumis, P.; Cuypers, J.;
   Sinachopoulos, D.; van Dessel, E.; Gal-Yam, A.; Papamastorakis, J.
2003A&A...402.1157N    Altcode:
  We present a catalog of secondary photometric standard stars in
  the neighborhood of 14 gravitationally lensed quasars. These stars
  were verified to be non variable using long-term monitoring. The
  instrumental magnitudes of the new standard stars have been transformed
  to the Johnson-Cousins BV(RI)<SUB>c</SUB> photometric system. For
  ten gravitational lenses (GLs) we also provide the BV(RI)<SUB>c</SUB>
  mean magnitudes of the integrated flux of all the lens components, for
  the epochs of the photometric calibration. <P />Based on observations
  made with a) the 1.0 m telescope at Wise Observatory, Israel, b)
  the 1.3 m telescope at Skinakas Observatory, Crete, Greece, and c)
  the 1.9 m SAAO telescope, Sutherland Observatory, South Africa. <P
  />Tables \ref{info}-\ref{colors-gls} and Fig. \ref{findingchart}
  are only available in electronic form at http://www.edpsciences.org

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Title: Digital Access to Aero- and Astrophotographic Archives
Authors: de Cuyper, J. -P.; van Dessel, E.; Pauwels, T.;
   Vanommeslaeghe, J.; Prils, H.; de Decker, G.; Pierre, O.; Lavreau,
   J.; Fernandez, M.; Tran, T.; Sterken, C.; David, M.; Schots, M.;
   Daelemans, G.
2003ASPC..295...93D    Altcode: 2003adass..12...93D
  The aim of this test-bed project, initiated and financed by the
  Belgian Federal Services for Scientific, Technical and Cultural
  Affairs (SSTC Project I2/AE/103), is to acquire within the coming
  4 years, the necessary know-how, hardware and software in order (i)
  to preserve the historic and the scientific information contained in
  aero- and astrophotographic archives, both on glass plates and on
  film; (ii) to provide a user-friendly intranet and internet access
  to the catalogue and the (meta)data; (iii) to make the photographic
  information exploitable again for scientific applications, by means
  of a high resolution digitisation technique.

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Title: Photometric Variability of the Gravitational Lens 0142-100
    (UM 673)
Authors: Sinachopoulos, D.; Nakos, Th.; Boumis, P.; van Dessel, E.;
   Burger, M.; Rodríguez-Gil, P.
2001AJ....122.1692S    Altcode: 2001astro.ph..7312S
  We present the results of a photometric CCD monitoring of the
  gravitational lens system UM 673 that took place from 1995 to 2000. In
  total, the doubly imaged quasar (QSO) was observed in the R band during
  29 photometric nights, using optical telescopes with dimensions in
  the range 0.6-1.3 m. We detected a significant variability in the
  total light of the UM 673 system, that is, in the light of the two
  QSO images plus the lensing galaxy. With respect to the magnitude of
  the gravitational lens system at its discovery, in 1986, UM 673 was
  0.3 mag brighter. Furthermore, our 1996 December measurements show
  that between 1995 November and 1997 October the system became even
  brighter, reaching a magnitude difference of 0.5 mag with respect to
  its discovery value. We also present R magnitudes and V-R colors of
  seven field stars situated in the vicinity of the lens, based on a 3.5
  month monitoring during the year 2000. Based on observations made with
  (1) the 60 cm Bochum and the ESO 90 cm Dutch telescopes, at La Silla,
  Chile, (2) the 1.2 m telescope at Kryonerion Observatory, Greece,
  (3) the 1.3 m telescope at Skinakas Observatory, Crete, Greece, and
  (4) the European Space Agency OGS telescope operated on the island of
  Tenerife by the Instituto de Astrofísica de Canarias in the Spanish
  Observatorio del Teide of the Instituto de Astrofísica de Canarias.

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Title: Photometric Variability of the gravitational lens UM 673
Authors: Sinachopoulos, D.; Nakos, T.; Boumis, P.; van Dessel, E.;
   Burger, M.; Rodriguez-Gil, P.
2001hell.confE.133S    Altcode:
  No abstract at ADS

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Title: Photometric Variability of UM 673
Authors: Sinachopoulos, D.; Nakos, T.; van Dessel, E.; Burger, M.
2001ASPC..237..101S    Altcode: 2001glrp.conf..101S
  No abstract at ADS

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Title: Surveys with the 4-m International Liquid Mirror Telescope
Authors: Poels, J.; Moreau, O.; Manfroid, J.; Surdej, J.; Borra, E.;
   Claeskens, J. F.; Jean, C.; Montfort, F.; Swings, J. P.; Vangeyte,
   B.; van Dessel, E.; Nakos, Th.
2001misk.conf..598P    Altcode:
  The working principle of liquid mirror telescopes (LMTs) is first
  reminded as well as their advantages and disadvantages over classical
  telescopes. For several obvious reasons (access to regions near the
  south galactic pole, galactic center, good image quality, ...),
  a best site location for such a LMT is somewhere in the Atacama
  desert. At latitudes near -22 - -29 degree, a deep (B = 24 mag.) LMT
  survey will approximately cover 90 square degrees at high galactic
  latitude, specially useful for gravitational lensing studies, for the
  identification of various classes of interesting extragalactic objects
  (cf. clusters, supernovae, etc. at high redshift) and subsequent
  follow-up observations with 8m-class telescopes. A short description
  of the handling of data products is also presented.

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Title: The Uccle Direct Astronomical Plate Archive Centre UDAPAC---A
    New International Facility for Inherited Observations
Authors: de Cuyper, J. -P.; Elst, E.; Hensberge, H.; Lampens, P.;
   Pauwels, T.; van Dessel, E.; Brosch, N.; Hudec, R.; Kroll, P.;
   Tsvetkov, M.
2001ASPC..238..125D    Altcode: 2001adass..10..125D
  An international facility to store, catalogue and digitise photographic
  plates is under development at the Royal Observatory of Belgium
  in Uccle-Brussels. The creation of such a facility requires a
  well-organized effort and substantial resources. However, the cost is
  not exorbitantly high if one takes advantage of the new generation of
  commercial, photogrammetric, flatbed scanners, which use the latest
  CCD technology. These scanners are relatively inexpensive, very fast,
  and comparable to dedicated scanners like PDS instruments in geometric
  and radiometric precision.

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Title: The 4-m International Liquid Mirror Telescope Project (ILMT)
Authors: Poels, J.; Borra, E.; Claeskens, J. F.; Jean, C.; Manfroid,
   J.; Montfort, F.; Moreau, O.; Nakos, Th.; Surdej, J.; Swings, J. P.;
   van Dessel, E.; Vangeyte, B.
2001ASPC..238...97P    Altcode: 2001adass..10...97P
  The working principle of liquid mirror telescopes (LMTs) is first
  reviewed along with their advantages and disadvantages over classical
  telescopes. For several reasons (access to regions near the south
  galactic pole, galactic center, good image quality, etc.), an excellent
  site for such an LMT is the Atacama desert. A deep (B~24 mag) LMT survey
  at latitudes near -22deg -- -29deg will cover ~90 square degrees at high
  galactic latitude and be especially useful for gravitational lensing
  studies, for the identification of various classes of interesting
  extragalactic objects (cf. clusters, supernovae, etc. at high redshift)
  and for subsequent follow-up observations with 8 m-class telescopes. A
  short description of the handling of data products is also presented.

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Title: UBV absolute CCD photometry and differential astrometry of
    a sample of visual double stars with A-type primaries
Authors: Shatsky, N.; Sinachopoulos, D.; Prado, P.; van Dessel, E.
1999A&AS..139...69S    Altcode:
  We present V magnitudes, (B-V) and (U-B) colours of the components of
  111 visual double stars and their relative position measurements rho and
  theta . The primaries are of spectral class A; the angular separation is
  in the 2farcs5 -8arcsec range. The observations were made at the 61-cm
  reflector of University of Toronto Southern Observatory, Chile. The
  obtained photometric results are of a moderate quality for absolute
  values (0.04() m (mag) in V and about 0.02() m in the (B-V) and (U-B)
  colour indices) and more precise in Delta V and Delta (U-B), Delta
  (B-V) (0.023() m and 0.015() m, respectively). We find that about 60%
  of secondaries are also of spectral type A; 56% of pairs have Delta
  (B-V) less than 0.1() m. The two-colour diagram reveals significant
  offset of objects from the curve of unreddened Main Sequence stars. A
  comprehensive survey of stars in the close vicinity to the objects
  is also presented. The final astrometric accuracy of ~ 0farcs01 in
  rho and 0fdg1 in theta provides additional measurements for study
  of relative motion of the components. Based on observations made at
  University of Toronto Southern Observatory, Las Campanas, Chile. Tables
  \arabic{tabptm}--\arabic{tabast} are only available in electronic form
  at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5)
  or via http://cdsweb.u-strasbg.fr/Abstract.html

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Title: CCD photometry and astrometry for visual double and multiple
    stars of the HIPPARCOS catalogue. I. Presentation of the large
    scale project
Authors: Oblak, E.; Lampens, P.; Cuypers, J.; Halbwachs, J. L.;
   Martín, E.; Seggewiss, W.; Sinachopoulos, D.; van Dessel, E. L.;
   Chareton, M.; Duval, D.
1999A&A...346..523O    Altcode: 1999astro.ph..4266O
  A description is given of the activities of an international
  working group created with the aim of obtaining both photometric and
  astrometric observations of visual double and multiple stars with
  angular separations in the range of one to fifteen arcseconds, that
  formed part of the HIPPARCOS Input Catalogue. The scientific aims and
  realisations of this European network are given. About 50 observational
  missions have been carried out in both hemispheres according to a
  pre-defined protocol. We describe the general and specifically designed
  methods used for the reduction of large amounts of CCD observations
  of double stars and give an outline of the results already presented
  and soon to be expected. Based on observations made at La Silla (ESO,
  Chile - Key Programme 7-009-49 K), Observatoire de Haute-Provence (OHP),
  Calar Alto (CLA), La Palma (LPL) and Jungfraujoch (JFJ) Observatories}

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Title: VizieR Online Data Catalog: UBV Astrometry and Photometry of
    doubles (Shatsky+, 1999)
Authors: Shatsky, N.; Sinachopoulos, D.; Prado, P.; van Dessel, E.
1999yCat..41390069S    Altcode:
  UBV CCD absolute photometry and differential astrometry of 111 southern
  visual binaries are presented. Observations have been performed at
  Las Campanas Observatory (Chile) in 1991-92 at 61-cm telescope. The
  separation range is 2.5-8arcsec. The mean epoch of the measurements
  is 1992.0. The photometry (table 1) was calibrated by one night of
  standard star observations. The positional parameters (table 3) are
  given in the reference system J2000 and calibrated using Hipparcos and
  CDS data. An additional table 2 provides the notes on observational
  circumstances. (3 data files).

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Title: CCD astrometry and instrumental Delta V photometry of visual
    double stars. V. Differential measurements of pairs with angular
    separations 1arcsec to 4arcsec
Authors: Sinachopoulos, D.; Dapergolas, A.; van Dessel, E.; Kontizas,
   E.
1999A&AS..136..525S    Altcode:
  We present angular separations, position angles and Delta V instrumental
  magnitude differences of 83 visual double stars with angular separations
  around two arcseconds. Our observations were made by means of a
  CCD detector attached to the Kryonerion 1.2 m telescope. 12 of
  them are common proper motion stars and their components should
  therefore be stars of common origin. Based on observations made
  at Kryonerion Observatory, Greece. Table 2 only available at the
  CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via
  http://cdsweb.u-strasbg.fr/Abstract.html}

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Title: VizieR Online Data Catalog: DeltaV photometry of visual double
    stars (Sinachopoulos+, 1999)
Authors: Sinachopoulos, D.; Dapergolas, A.; van Dessel, E.; Kontizas,
   E.
1999yCat..41360525S    Altcode:
  We present angular separations, position angles and ΔV instrumental
  magnitude differences of 83 visual double stars with angular separations
  around two arcseconds. Our observations were made by means of a CCD
  detector attached to the Kryonerion 1.2m telescope. 12 of them are
  common proper motion stars and their components should therefore be
  stars of common origin. (1 data file).

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Title: CCD astrometry and UBV photometry of visual
    binaries. II. Visual double stars with mainly G - type primaries
    and relatively small angular separation
Authors: Sinachopoulos, D.; van Dessel, E.
1998A&AS..130..299S    Altcode:
  Differences Delta V of magnitude and Delta (B-V) and Delta (U-B)
  colours, as well as separations and position angles of 42 relatively
  close double stars are presented. The selection criteria of our sample
  are: the relatively small separation (between 2.5 and 5 arcseconds),
  magnitude difference under 1.25 mag, and mainly G-type primaries. The
  CCD observations, performed at the 90 cm Dutch telescope at ESO,
  were made using the Bessel U, B and V filters; the astrometry was
  done in the V filter only. From the analysis of the photometric
  data we conclude that 16 binaries in our sample have components with
  practically the same T_eff, since they have almost the same colours;
  one binary has components with identical characteristics. We also note
  the good internal accuracy of the astrometric CCD measurements. Based
  on observations made at ESO La Silla, Chile.

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Title: A list of Hipparcos very wide visual double stars for the
    astrometric calibration of imaging with CCDs
Authors: Sinachopoulos, Dimitrios; van Dessel, Edwin; Geffert, Michael
1998AcHA....3..195S    Altcode:
  We have selected from the Hipparcos catalogue (ESA 1997) a list
  of 307 very wide visual double stars, which can be used for
  performing an accurate astrometric calibration of CCD detectors
  mounted on telescopes. Angular separations are between 10 and
  100 arcsec, mainly around 20 arc seconds and less than 35 arc
  seconds. Our list can be obtained from the Internet at the address
  http://midas.oma.be/www_root/serverdoc/www/ccdlas.html or it can
  be obtained from the authors directly. All information in our
  list was extracted, or computed from the Hipparcos catalogue. The
  format is simple containing one line per visual double star. (RA,
  Dec) coordinates of the component with the smallest RA value are
  given first. This component is obviously not always the primary. The
  epoch of the coordinates is the Hipparcos one: 1995.25. The following
  columns give V magnitudes and (B-V) colours of both components, their
  angular separation, and Hipparcos identifiers (HIC numbers). For
  the information that will enable you to compute the current value
  of the angular separation of each wide visual double star used for
  calibration, you have to search in the main Hipparcos catalogue. Each
  component of the double stars in our list has a separate entry in
  this catalogue. According to Sinachopoulos and van Dessel (1998), the
  Hipparcos catalogue contains some erroneous entries for wide visual
  double stars components as well. For this reason, it is advised to
  use at least three double stars of the list each time you calibrate
  your detector. All double stars in our list have been introduced to
  the Hipparcos mission by Brosche and Sinachopoulos (1988, 1989). In
  case you get problems or doubts on the correctness of the Hipparcos
  results for a particular double star, you can use information of these
  two publications for an additional control.

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Title: EIT Observations of the Extreme Ultraviolet Sun
Authors: Moses, D.; Clette, F.; Delaboudinière, J. -P.; Artzner,
   G. E.; Bougnet, M.; Brunaud, J.; Carabetian, C.; Gabriel, A. H.;
   Hochedez, J. F.; Millier, F.; Song, X. Y.; Au, B.; Dere, K. P.; Howard,
   R. A.; Kreplin, R.; Michels, D. J.; Defise, J. M.; Jamar, C.; Rochus,
   P.; Chauvineau, J. P.; Marioge, J. P.; Catura, R. C.; Lemen, J. R.;
   Shing, L.; Stern, R. A.; Gurman, J. B.; Neupert, W. M.; Newmark,
   J.; Thompson, B.; Maucherat, A.; Portier-Fozzani, F.; Berghmans, D.;
   Cugnon, P.; Van Dessel, E. L.; Gabryl, J. R.
1997SoPh..175..571M    Altcode:
  The Extreme Ultraviolet Imaging Telescope (EIT) on board the SOHO
  spacecraft has been operational since 2 January 1996. EIT observes
  the Sun over a 45 x 45 arc min field of view in four emission line
  groups: Feix, x, Fexii, Fexv, and Heii. A post-launch determination
  of the instrument flatfield, the instrument scattering function, and
  the instrument aging were necessary for the reduction and analysis
  of the data. The observed structures and their evolution in each
  of the four EUV bandpasses are characteristic of the peak emission
  temperature of the line(s) chosen for that bandpass. Reports on the
  initial results of a variety of analysis projects demonstrate the range
  of investigations now underway: EIT provides new observations of the
  corona in the temperature range of 1 to 2 MK. Temperature studies of
  the large-scale coronal features extend previous coronagraph work
  with low-noise temperature maps. Temperatures of radial, extended,
  plume-like structures in both the polar coronal hole and in a low
  latitude decaying active region were found to be cooler than the
  surrounding material. Active region loops were investigated in detail
  and found to be isothermal for the low loops but hottest at the loop
  tops for the large loops.

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Title: EIT and LASCO Observations of the Initiation of a Coronal
    Mass Ejection
Authors: Dere, K. P.; Brueckner, G. E.; Howard, R. A.; Koomen, M. J.;
   Korendyke, C. M.; Kreplin, R. W.; Michels, D. J.; Moses, J. D.;
   Moulton, N. E.; Socker, D. G.; St. Cyr, O. C.; Delaboudinière, J. P.;
   Artzner, G. E.; Brunaud, J.; Gabriel, A. H.; Hochedez, J. F.; Millier,
   F.; Song, X. Y.; Chauvineau, J. P.; Marioge, J. P.; Defise, J. M.;
   Jamar, C.; Rochus, P.; Catura, R. C.; Lemen, J. R.; Gurman, J. B.;
   Neupert, W.; Clette, F.; Cugnon, P.; Van Dessel, E. L.; Lamy, P. L.;
   Llebaria, A.; Schwenn, R.; Simnett, G. M.
1997SoPh..175..601D    Altcode:
  We present the first observations of the initiation of a coronal mass
  ejection (CME) seen on the disk of the Sun. Observations with the EIT
  experiment on SOHO show that the CME began in a small volume and was
  initially associated with slow motions of prominence material and a
  small brightening at one end of the prominence. Shortly afterward,
  the prominence was accelerated to about 100 km s<SUP>-1</SUP> and
  was preceded by a bright loop-like structure, which surrounded an
  emission void, that traveled out into the corona at a velocity of
  200-400 km s<SUP>-1</SUP>. These three components, the prominence,
  the dark void, and the bright loops are typical of CMEs when seen at
  distance in the corona and here are shown to be present at the earliest
  stages of the CME. The event was later observed to traverse the LASCO
  coronagraphs fields of view from 1.1 to 30 R⊙. Of particular interest
  is the fact that this large-scale event, spanning as much as 70 deg in
  latitude, originated in a volume with dimensions of roughly 35" (2.5
  x 10<SUP>4</SUP> km). Further, a disturbance that propagated across
  the disk and a chain of activity near the limb may also be associated
  with this event as well as a considerable degree of activity near the
  west limb.

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Title: UBV absolute CCD photometry and differential astrometry of
    close visual double stars, with G-type primaries
Authors: Nakos, T.; Sinachopoulos, D.; van Dessel, E.
1997A&AS..124..353N    Altcode:
  We present V magnitudes, (B-V) and (U-B) colours of close visual
  double star components, and their differences as well as separations
  and position angles of 40 visual double stars. The common properties
  of the members of this sample are the small angular separation rho,
  which is less than 7”, and the common spectral type of the primaries,
  which are of G-type. The observations made with the Bessel U, B and V
  filters, while the astrometry was performed in the V filter only. For
  the observations, the CCD camera attached to the Cassegrain focus of
  the 90 cm Dutch telescope, at La Silla, Chile, had been used. From the
  analysis of the data we concluded that from the sample of the fourty
  double stars observed seven proved to be physical pairs, while the rest
  must have common origin components. Based on observations made at ESO
  La Silla, Chile. Tables 1 and 2 are only available in electronic form
  at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5)
  or via http://cdsweb.u-strasbg.fr/Abstract.html

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Title: Imaging the solar corona in the EUV
Authors: Delaboudiniere, J. -P.; Stern, R. A.; Maucherat, A.;
   Portier-Fozzani, F.; Neupert, W. M.; Gurman, J. B.; Catura, R. C.;
   Lemen, J. R.; Shing, L.; Artzner, G. E.; Brunaud, J.; Gabriel, A. H.;
   Michels, D. J.; Moses, J. D.; Au, B.; Dere, K. P.; Howard, R. A.;
   Kreplin, R.; Defise, J. M.; Jamar, C.; Rochus, P.; Chauvineau, J. P.;
   Marioge, J. P.; Clette, F.; Cugnon, P.; van Dessel, E. L.
1997AdSpR..20.2231D    Altcode:
  The SOHO (SOlar and Heliospheric Observatory) satellite was launched on
  December 2nd 1995. After arriving at the Earth-Sun (L1) Lagrangian point
  on February 14th 1996, it began to continuously observe the Sun. As
  one of the instruments onboard SOHO, the EIT (Extreme ultraviolet
  Imaging Telescope) images the Sun's corona in 4 EUV wavelengths. The
  He II filter at 304 A˚ images the chromosphere and the base of the
  transition region at a temperature of 5 - 8 x 10^4 K; the Fe IX-X
  filter at 171 A˚ images the corona at a temperature of ~ 1.3 x 10^6 K;
  the Fe XII filter at 195 A˚ images the quiet corona outside coronal
  holes at a temperature of ~ 1.6 x 10^6 K; and the Fe XV filter at 284
  A˚ images active regions with a temperature of ~ 2.0 x 10^6 K. About
  5000 images have been obtained up to the present. In this paper,
  we describe also some aspects of the telescope and the detector
  performance for application in the observations. Images and movies
  of all the wavelengths allow a look at different phenomena present in
  the Sun's corona, and in particular, magnetic field reconnection.

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Title: First Results from EIT
Authors: Clette, F.; Delaboudiniere, J. -P.; Artzner, G. E.; Brunaud,
   J.; Gabriel, A. H.; Hochedez, J. -F.; Millier, F.; Song, X. Y.; Au, B.;
   Dere, K. P.; Howard, R. A.; Kreplin, R.; Michels, D. J.; Moses, J. D.;
   Defise, J. -M.; Jamar, C.; Rochus, P.; Chauvineau, J. -P.; Marioge,
   J. -P.; Catura, R. C.; Lemen, J. R.; Shing, L.; Stern, R. A.; Gurman,
   J. B.; Neupert, W. M.; Maucherat, A.; Cugnon, P.; van Dessel, E. L.
1997ASPC..118..268C    Altcode: 1997fasp.conf..268C
  The Extreme-UV Imaging telescope has already produced more than 15000
  wide-field images of the corona and transition region, on the disk
  and up to 1.5R_⊙ above the limb, with a pixel size of 2.6\arcsec. By
  using four different emission lines, it provides the global temperature
  distribution in the quiet corona, in the range 0.5 to 3*E(6) K. Its
  excellent sensitivity and wide dynamic range allow unprecedented views
  of low emission features, even inside coronal holes. Those so-called
  “quiet” regions actually display a wide range of dynamical phenomena,
  in particular at small spatial scales and at time scales going down
  to only a few seconds, as revealed by all EIT time sequences of
  full- or partial-field images. The initial results presented here
  demonstrate the importance of this wide-field imaging experiment for
  a good coordination between SOHO and ground-based solar telescopes,
  as well as for science planning.

---------------------------------------------------------
Title: UBV photometry of wide visual double stars. V. Double stars
    with mainly K- and M- type primaries.
Authors: Sinachopoulos, D.; van Dessel, E. L.
1996A&AS..119..483S    Altcode:
  We present UBV photometric observations of 55 wide visual double stars
  with K- and M- type primaries. Our observations have been compared and
  combined with information available in the literature. At least 58%
  of them are optical pairs.

---------------------------------------------------------
Title: VizieR Online Data Catalog: CCD UBV photometry of close visual
    doubles (Nakos+ 1997)
Authors: Nakos, T.; Sinachopoulos, D.; van Dessel, E.
1996yCat..41240353N    Altcode:
  We present V magnitudes, (B-V) and (U-B) colours of close visual
  double star components, and their differences as well as separations
  and position angles of 40 visual double stars. The common properties
  of the members of this sample are the small angular separation ρ,
  which is less than 7", and the common spectral type of the primaries,
  which are of G-type. The observations made with the Bessel U, B and V
  filters, while the astrometry was performed in the V filter only. For
  the observations, the CCD camera attached to the Cassegrain focus of
  the 90 cm Dutch telescope, at La Silla, Chile, had been used. From the
  analysis of the data we concluded that from the sample of the fourty
  double stars observed seven proved to be physical pairs, while the
  rest must have common origin components. (3 data files).

---------------------------------------------------------
Title: VizieR Online Data Catalog: UBV photometry of double
    stars. (Sinachopoulos+ 1996)
Authors: Sinachopoulos, D.; van Dessel, E. L.
1996yCat..41190483S    Altcode:
  We present UBV photometric observations of 55 wide visual double stars
  with K- and M- type primaries. Our observations have been compared and
  combined with information available in the literature. At least 58%
  of them are optical pairs. (2 data files).

---------------------------------------------------------
Title: VizieR Online Data Catalog: VRI photometry of wide double stars
    (Sinachopoulos+ 1995)
Authors: Sinachopoulos, D.; Cuypers, J.; Lampens, P.; Oblak, E.;
   van Dessel, E. L.
1996yCat..41120291S    Altcode:
  We are presenting VRI photometry of 93 wide visual double stars
  having late B- or A- type primaries, taken from the Annex of Double
  and Multiple Stars of the HIPPARCOS Input Catalogue. Spectral types
  have been estimated for most of the primaries and for the majority of
  the secondaries. 40% of them probably have common origin components,
  for which we calculated photometric parallaxes and some orbital values
  estimates. (4 data files).

---------------------------------------------------------
Title: Old and new on A0535+26 / HDE 245770.
Authors: Burger, M.; van Dessel, E. L.; Giovannelli, F.;
   Sabau-Graziati, L.; Bartolini, C.; Guarnieri, A.; Piccioni, A.
1996MmSAI..67..365B    Altcode:
  No abstract at ADS

---------------------------------------------------------
Title: Photometric Monitoring Of The Lensed QSO 0957+561
Authors: Sinachopoulos, D.; Burger, M.; van Dessel, E.; Geffert, M.;
   Thibor, M.; Colin, J.; Ducourant, Ch.
1996IAUS..173...53S    Altcode:
  No abstract at ADS

---------------------------------------------------------
Title: EIT: Extreme-Ultraviolet Imaging Telescope for the SOHO Mission
Authors: Delaboudinière, J. -P.; Artzner, G. E.; Brunaud, J.; Gabriel,
   A. H.; Hochedez, J. F.; Millier, F.; Song, X. Y.; Au, B.; Dere, K. P.;
   Howard, R. A.; Kreplin, R.; Michels, D. J.; Moses, J. D.; Defise,
   J. M.; Jamar, C.; Rochus, P.; Chauvineau, J. P.; Marioge, J. P.;
   Catura, R. C.; Lemen, J. R.; Shing, L.; Stern, R. A.; Gurman, J. B.;
   Neupert, W. M.; Maucherat, A.; Clette, F.; Cugnon, P.; Van Dessel,
   E. L.
1995SoPh..162..291D    Altcode:
  The Extreme-ultraviolet Imaging Telescope (EIT) will provide wide-field
  images of the corona and transition region on the solar disc and up to
  1.5 R⊙ above the solar limb. Its normal incidence multilayer-coated
  optics will select spectral emission lines from Fe IX (171 å), Fe
  XII (195 å), Fe XV (284 å), and He II (304 å) to provide sensitive
  temperature diagnostics in the range from 6 × 10<SUP>4</SUP> K to 3
  × 10<SUP>6</SUP> K. The telescope has a 45 x 45 arcmin field of view
  and 2.6 arcsec pixels which will provide approximately 5-arcsec spatial
  resolution. The EIT will probe the coronal plasma on a global scale,
  as well as the underlying cooler and turbulent atmosphere, providing
  the basis for comparative analyses with observations from both the
  ground and other SOHO instruments. This paper presents details of the
  EIT instrumentation, its performance and operating modes.

---------------------------------------------------------
Title: VRI photometry of wide double stars with A- type primaries.
Authors: Sinachopoulos, D.; Cuypers, J.; Lampens, P.; Oblak, E.;
   van Dessel, E. L.
1995A&AS..112..291S    Altcode:
  We are presenting VRI photometry of 93 wide visual double stars
  having late B- or A- type primaries, taken from the Annex of Double
  and Multiple Stars of the HIPPARCOS Input Catalogue. Spectral types
  have been estimated for most of the primaries and for the majority of
  the secondaries. 40% of them probably have common origin components,
  for which we calculated photometric parallaxes and some orbital values
  estimates.

---------------------------------------------------------
Title: CCD astrometry and instrumental {DELTA}V photometry of wide
    visual double stars. IV. Differential measurements of northern pairs.
Authors: Nakos, T.; Sinachopoulos, D.; van Dessel, E.
1995A&AS..112..453N    Altcode:
  We present relative positions and instrumental visual magnitude
  differences ({DELTA}V) of 101 northern wide double star components. The
  mean accuracy of the magnitude differences is 0.01 magnitudes, of
  the angular separation 0.04 arcseconds, and of position angle 0.13
  degrees. Most of the programme pairs are targets of the HIPPARCOS
  mission and they have been often observed during the last 150 years.

---------------------------------------------------------
Title: CCD astrometry and instrumental (Delta)V photometry of wide
    visual double stars. III. Differential measurements of often observed
    southern pairs.
Authors: van Dessel, E.; Sinachopoulos, D.
1993A&AS..100..517V    Altcode:
  We present accurate relative positions and instrumental visual (Bessel
  V) magnitude differences of southern wide star components. The mean
  accuracy of the angular separation is 0.02 arcsecs, which corresponds
  to 1.5 micron on the CCD chip, and of magnitude difference 0.007
  mag/exposure. The program pairs are targets of the HIPPARCOS mission
  and they have been observed at least four times in the last 150 yrs.

---------------------------------------------------------
Title: A photometric study of wide visual double stars. IV. UVBY
    photometry of wide visual double stars with G-type primaries.
Authors: Sinachopoulos, D.; van Dessel, E.
1993A&AS...98...17S    Altcode:
  We performed uvby aperture photometry of wide visual double stars with
  G-type primaries. The minimum angular separation of the components is
  10 arcsecs and mainly less than 20 arcsecs. As both components have
  often similar photometric and astrophysical parameters, we infer that
  most of these double stars have components of common origin.

---------------------------------------------------------
Title: Photometry of Close Visual Binaries
Authors: Oblak, E.; Argue, A. N.; Brosche, P.; Cuypers, J.; Dommanget,
   J.; Duquennoy, A.; Froeschle, M.; Grenon, M.; Halbwachs, J. L.;
   Jasniewicz, C.; Lampens, P.; Martin, F.; Mermilliod, J. C.; Mignard,
   F.; Sinachopoulos, D.; Seggewiss, W.; van Dessel, E.
1993ppsp.conf..139O    Altcode: 1993IAUCo.136P.139O
  No abstract at ADS

---------------------------------------------------------
Title: The use of Expert Systems in astronomical data handling.
Authors: Sinachopoulos, D.; Sinachopoulos, A.; van Dessel, E.
1993ESOC...47..209S    Altcode: 1993daan.work..209S
  Numerical instabilities are a common problem in least square fitting of
  mathematical functions to observational data. Procedures corresponding
  to the expert systems method can then be very helpful. Expert Systems
  are computer programs offerring problem solving methods based on facts
  and rules which formalize the knowledge on special topics. The idea
  behind such expert system programs is that the users, the "experts",
  know the possible limit values of the variables to be determined by
  the least square fitting.

---------------------------------------------------------
Title: Solar corona synoptic observations from SOHO with an Extreme
    Ultraviolet Imaging Telescope.
Authors: Delaboudinière, J. P.; Gabriel, A. H.; Artzner, G. E.;
   Dere, K.; Howard, R.; Michels, D.; Catura, R.; Lemen, J.; Stern, R.;
   Gurman, J.; Neupert, W.; Cugnon, P.; Koeckelenbergh, A.; van Dessel,
   E. L.; Jamar, C.; Maucherat, A.
1992ESASP.348...21D    Altcode: 1992cscl.work...21D
  The major scientific objective of the EUV Imaging Telescope (EIT)
  is to study the evolution of coronal structure over a wide range
  of spatial and temporal scales and temperatures. A second strategic
  objective is to provide full disk synoptic maps of the global corona
  to aid in unifying SOHO (Solar and Heliospheric Observatory)/Cluster
  investigations. EIT will also provide images to support the planning
  of detailed spectroscopic investigations by the CDS (Coronal Diagnostic
  Spectrometer) and SUMER spectrometers in SOHO. EIT observations will be
  made in four narrow spectral bands, centered at 171 A (Fe 9), 195 A(Fe
  12), 284 A (Fe 15), and 304 A (He 2) representing restricted temperature
  domains within a wide temperature range from 40,000 to 3,000,000
  K. The results will be images of the solar atmosphere from the upper
  chromosphere and transition region to the active region corona. These
  maps, made at appropriate time intervals, will be used to study the fine
  structures in the solar corona and to relate their dynamic properties
  to the underlying chromosphere and photosphere. Dynamic events in the
  inner corona will be related to white light transients in the outer
  corona, and observations of the internal structure of coronal holes
  will be used to investigate origins of the solar wind.

---------------------------------------------------------
Title: CCD and conventional photometry of components of visual
    binaries.
Authors: Oblak, E.; Argue, A. N.; Brosche, P.; Cuypers, J.; Dommanget,
   J.; Duquennoy, A.; Froeschlé, M.; Grenon, M.; Halbwachs, J. L.;
   Jasniewicz, G.; Lampens, P.; Martin, E.; Mermilliod, J. C.; Mignard,
   F.; Sinachopoulos, D.; Seggewiss, W.; van Dessel, E.
1992Msngr..69...14O    Altcode:
  No abstract at ADS

---------------------------------------------------------
Title: An Impression from Programmes Performed at ESO about the
    Interest of European Astronomers in Visual Double and Multiple
    Star Research
Authors: van Dessel, E. L.
1992ASPC...32..259V    Altcode: 1992IAUCo.135..259V; 1992cadm.conf..259V
  No abstract at ADS

---------------------------------------------------------
Title: The European Network of Laboratories: Visual Double Stars
Authors: Oblak, E.; Argue, A. N.; Brosche, P.; Cuypers, J.; Dommanget,
   J.; Duquennoy, A.; Froeschle, M.; Grenon, M.; Haibwachs, J. -L.;
   Jasniewicz, G.; Lampens, P.; Mermilliod, J. C.; Mignard, F.;
   Sinachopoulos, D.; Seggewiss, W.; van Dessel, E.
1992ASPC...32..454O    Altcode: 1992IAUCo.135..454O; 1992cadm.conf..454O
  No abstract at ADS

---------------------------------------------------------
Title: Stromgren Photometry of Wide Visual Double Stars with G-type
    Primaries, Most of Which Have Common Origin Components
Authors: Sinachopoulos, D.; van Dessel, E.
1992ASPC...32..355S    Altcode: 1992IAUCo.135..355S; 1992cadm.conf..355S
  No abstract at ADS

---------------------------------------------------------
Title: UBV CCD Photometry and Astrometry of "Close" Visual Double
    Stars
Authors: van Dessel, E.; Sinachopoulos, D.; Prado, P.
1992ASPC...32..362V    Altcode: 1992cadm.conf..362V; 1992IAUCo.135..362V
  No abstract at ADS

---------------------------------------------------------
Title: High precision radial velocity determinations for the study
    of the internal kinematical and dynamical structure and evolution
    of young stellar groups.
Authors: Hensberge, H.; van Dessel, E. L.; Burger, M.; de Zeeuw,
   P. T.; Lub, J.; Lepoole, R. S.; Verschueren, W.; David, M.; Theuns,
   T.; De Loore, C.; de Geus, E. J.; Mathieu, R. D.; Blaauw, A.
1990Msngr..61...20H    Altcode:
  No abstract at ADS

---------------------------------------------------------
Title: Multifrequency behaviour of the X-ray/Be system A 0535 +
    26/HDE 245770 at the perioastron passage in March/April 1989
Authors: Giovannelli, F.; Persi, P.; de Martino, D.; Bartolini,
   C.; Guarnieri, A.; Piccioni, A.; Teoderani, M.; Burger, M.; van
   Dessel, E. L.; Kurt, V. G.; Sheffer, E. K.; Waters, L. B.; Gonzalez
   Martinez-Pais, I.; Gnedin, Y. N.; Larionov, V. M.; Shakovskaya, N. I.;
   Dapergolas, A.; Kontizas, E.
1990ESASP.310..379G    Altcode: 1990eaia.conf..379G
  No abstract at ADS

---------------------------------------------------------
Title: Fourteen Years of Multifrequency Coordinated Observations of
the X-Ray / BE System A:0535+26 / HDE245770
Authors: Giovannelli, F.; Bartolini, C.; Guarnieri, A.; Piccioni,
   A.; Burger, M.; van Dessel, E. L.; Kurt, V. G.; Sheffer, E. K.; de
   Martino, D.; Waters, R.; Martinez-Pais, I. Gonzalez; Gnedin, Yu. N.;
   Larionov, V. M.; Shakovskaya, N. I.
1990Ap&SS.169..139G    Altcode:
  Within the framework of a very long multifrequency campaign of
  coordinated, and very often simultaneous, observations of the transient
  X-ray/Be system A 0535+26/HDE 245770, we present a summary of this
  large collection of data taken with IUE and ASTRON satellites as well
  as with many ground-based telescopes in optical and IR regions. In
  this paper we emphasize the study of the physics and dynamics of the
  mass transfer at periastron and subsequent X-ray flaring, which is a
  typical problem of the X-ray/Be binary system class.

---------------------------------------------------------
Title: Extreme ultraviolet imaging telescope on board the Solar
    Heliospheric Observatory
Authors: Delaboudiniere, Jean-Pierre; Gabriel, Alan H.; Artzner,
   Guy E.; Millier, F.; Michels, Donald J.; Dere, Kenneth P.; Howard,
   Russell A.; Kreplin, Robert W.; Catura, Richard C.; Stern, Robert A.;
   Lemen, James R.; Neupert, Werner M.; Gurman, Joseph B.; Cugnon, P.;
   Koeckelenbergh, A.; van Dessel, E. L.; Jamar, Claude A.; Maucherat,
   Andre J.; Chauvineau, Jean-Pierre; Marioge, Jean-Paul
1989SPIE.1160..518D    Altcode: 1989xeoa.conf..518D
  The design of the multibandpass Extreme-Ultraviolet Imaging Telescope
  designed for 1996 launch on board the Solar Heliospheric Observatory
  is described. The telescope will observe simultaneously distinct
  temperature ranges in the solar corona, defined by well chosen emission
  lines. Images in four narrow bandpasses at wavelengths ranging from 17
  to 31 nm will be obtained using normal-incidence multilayered optics
  deposited on quadrants of a Ritchey-Chretien telescope. Results are
  presented on the performances measured on a 2/3 scale mock-up. The
  bandpasses could be adjusted to better than 1 percent in wavelength.

---------------------------------------------------------
Title: A 0535+26/HD 245770 - A typical Be/X-ray transient system :
    coordinated multiwavelength twelve years monitor.
Authors: Giovannelli, F.; Burger, M.; van Dessel, E. L.; Bartolini,
   C.; Guarnieri, A.; Piccioni, A.; Kurt, V. G.; Sheffer, E. K.
1988ESASP.281a.141G    Altcode: 1988uvai....1..141G; 1988IUE88...1..141G
  The transient X-ray binary system A 0535+26/HDE 245770 was monitored
  at different wavelengths since its discovery as X-ray emitter. These
  coordinated observations reveal correlations in the variability of the
  optical and X-ray emissions. During activity periods of the system, UV
  discrete absorption components in Si IV and C IV resonance lines whose
  velocities vary between -300 and -600 km/sec were detected. The study
  of the narrow absorption components at the expected activity epochs
  (periastron passages of the neutron star) simultaneously with X-ray,
  optical, and IR observations is essential for a better knowledge of
  the wind structure of the Be star and its interaction with the neutron
  star. The physics and dynamics of mass transfer at periastron and
  subsequent X-ray flaring, are emphasized.

---------------------------------------------------------
Title: Wide components in double and multiple stars
Authors: Dommanget, J.; van Dessel, E. L.; Kopal, Zdenek
1988Ap&SS.142.....D    Altcode: 1988IAUCo..97.....D
  Papers are presented on the concept of star multiplicity, the
  photometric cataloging of visual and multiple stellar systems, the
  cataloging of ephemerides and apparent orbits for visual binaries,
  and a search for wide pairs among nearby stars. Also considered are
  distant companions in double and multiple stars, the kinematics of
  trapezium-type systems, the classification of multiple systems in the
  general field, and photoelectric observations of CPM stars in the BVRI
  system. Other topics include the frequency of wide binaries among the
  southern barium stars, statistical studies on wide pairs, theoretical
  models for wide binary evolution, and evidence of mass loss in visual
  binary stars.

---------------------------------------------------------
Title: Wide components in double and multiple stars. Proceedings of
    the 97thColloquium of the International Astronomical Union, held in
    Brussels,Belgium, 8 - 13 June 1987.
Authors: Dommanget, J.; van Dessel, E. L.; Kopal, Z.; Melchior, P.
1988wcdm.book.....D    Altcode:
  No abstract at ADS

---------------------------------------------------------
Title: The Be/X-RAY System HDE 245770/A0535+26 in an Active Phase
Authors: Bartolini, C.; Burger, M.; van Dessel, E. L.; Giovannelli,
   F.; Guarnieri, A.; De Loore, C.; Piccioni, A.
1987pbes.coll..309B    Altcode: 1987IAUCo..92..309B
  The authors report on the sudden appearance and disappearance
  of (mainly) Fe II emission lines in the Be/X-ray system HDE
  245770/A0535+26, about 24 days before an X-ray outburst was observed.

---------------------------------------------------------
Title: X-Ray Ultraviolet and Optical Monitoring of the X-Ray /
BE Transient System A:0535+26 / HDE245770
Authors: Giovannelli, F.; van Dessel, E. L.; Burger, M.; De Loore, C.;
   Bartolini, C.; Guarnieri, A.; Piccioni, A.; Golynskaya, I. M.; Kurt,
   V. G.; Mizyakina, T. A.; Shafer, E. Y.; Shamolin, V. M.; Sheffer,
   E. K.; Smirnoff, A. S.
1986ESASP.263..459G    Altcode: 1986NIA86......459G; 1986niia.conf..459G
  The X-ray/Be transient system A 0535+26/HDE 245770 was monitored
  in X-ray, UV, and optical wavelengths to study the lighting of X-ray
  outbursts. The X-ray observations were carried out with ASTRON satellite
  on April 19, 1985 and March 17, 1986, dates of expected X-ray outbursts
  as predicted by the 111 day orbital periodicity. The measured fluxes
  are 6.5 mCrab and less than 5 mCrab in April 1985 and March 1986,
  respectively. The IUE observations were performed on January 29,
  and on March 13 and 15, 1986, predicted periods of quiescence and
  a bit earlier than an outburst, respectively. Optical spectroscopic
  observations were performed too. The absence of two X-ray expected
  outbursts implies either an inaccuracy of 111 day period or a temporary
  turning-off of the source.

---------------------------------------------------------
Title: The transient X-ray source A 0535+26: coordinated observations
    in X-ray, UV, optical and IR regions.
Authors: Giovannelli, F.; Ferrari Toniolo, M.; Persi, P.; Golinskaya,
   I. M.; Golynskaya, I. M.; Kurt, V. G.; Mizyakina, T. A.; Shafer,
   E. Yu.; Shamolin, V. M.; Smirnoff, A. S.; Smirnov, A. S.; Sheffer,
   E. K.; Zaytzeva, G. V.; Zajtseva, G. V.; van Dessel, E. L.; van Diest,
   H.; Hensberge, H.; Burger, M.; De Loore, C.; Bartolini, C.; Guarnieri,
   A.; Lolli, M.; Piccioni, A.; Gnedin, Yu. N.; Khozov, G. V.; Larionov,
   V. M.; Shakovskaya, N. I.; Shakhovskaya, N. I.
1985xra..conf..205G    Altcode: 1984xra..conf..205G
  Multispectral coordinated observations of the Be/X-ray binary HDE
  245770/A 0535+26 are briefly presented and discussed. A strong X-ray
  event was revealed and the period of the X-ray pulsar measured during
  a quiescent phase.

---------------------------------------------------------
Title: Multispectral analysis in the UV, optical and IR of HDE 245770
    = A 0535+26.
Authors: De Loore, C.; Giovannelli, F.; van Dessel, E. L.; Bartolini,
   C.; Burger, M.; Ferrari-Toniolo, M.; Giangrande, A.; Guarnieri, A.;
   Hellings, P.; Hensberge, H.; Persi, P.; Piccioni, A.; van Diest, H.
1984A&A...141..279D    Altcode:
  The characteristics of the Be/X-ray binary system HDE 245770/A0535+26
  are examined from UV, visual, IR and X-ray data. A sequence of
  observations in the optical preceding an X-ray outburst is interpreted
  as the ejection of a shell by the Be primary. An evolutionary scenario
  is presented that produces a system like HDE 245770. An effective
  temperature of 26000±2000K is derived for the Be star. The mass loss
  rate through stellar wind from the primary is determined. The Be star
  is not filling its Roche lobe and there is no accretion disk around
  the compact companion. The system configuration can be simulated
  with an evolution code allowing for the simultaneous evolution of two
  components - a 20 M_sun; primary and a 15 M_sun; secondary - producing
  Be/X-ray binaries of this kind, with systems like φ Per as progenitor.

---------------------------------------------------------
Title: Coordinated X-ray, ultraviolet, optical, and infrared
    observations ofthe transient source A0535+26.
Authors: Giovannelli, F.; Ferrari-Toniolo, M.; Persi, P.; Bartolini,
   C.; Guarnieri, A.; Piccioni, A.; van Dessel, E. L.; Burger, M.;
   de Loore, C.; Bisnovatyi-Kogan, G. S.; Bisnovatyj-Kogan, G. S.;
   Golynskaya, I. M.; Kurt, V. G.; Mizyakina, T. A.; Shafer, E. Yu.;
   Shamolin, V. M.; Sheffer, E. K.; Smirnoff, A. S.; Smirnov, A. S.
1984ESASP.218..439G    Altcode: 1984iue..conf..439G
  Data of A 0535+26/HDE 245770 from IR, optical, UV and X wavelengths
  before and after one of the strongest X-ray outbursts, expected on
  the basis of the 111-day periodicity of this source and detected
  by the ASTRON satellite on February 1, 1984 are presented. The IUE
  observations performed on Nov 10, 1983 and Jan 23, 1984 are entirely
  compatible with earlier measurements. Optical spectra taken immediately
  before the X-ray outburst show H gamma in absorption and H alpha in
  weakened emission. In September and in January 1984 before the X-ray
  outburst the star presents diminished IR excess. Mass loss is discussed.

---------------------------------------------------------
Title: New orbital elements for the visual binary IDS 14527 S 2715 =
    ADS 9453.
Authors: van Dessel, E.
1983BAORB...9..254V    Altcode:
  No abstract at ADS

---------------------------------------------------------
Title: New orbital elements for the visual binary IDS 14527 S 2715 =
    ADS 9453.
Authors: van Dessel, E.
1983BuAst...9..254V    Altcode:
  No abstract at ADS

---------------------------------------------------------
Title: The observation of radial velocities of visual binaries
Authors: van Dessel, E.; Dommanget, J.
1982BICDS..23..106V    Altcode:
  No abstract at ADS

---------------------------------------------------------
Title: Ultraviolet, optical, and infrared observations of HDE
    245770/A 0535+26.
Authors: Giovannelli, F.; De Loore, C.; Bartolini, C.; Burger,
   M.; Ferrari-Toniolo, M.; Giangrande, A.; Guarnieri, A.; Persi, P.;
   Piccioni, A.; van Dessel, E. L.
1982ESASP.176..233G    Altcode: 1982iue..conf..233G; 1982IUE3r......233G
  Observations of the Be X-ray source A 0535 + 26 are described. The
  features of the source changed notably between Feb. and Oct. 1981:
  the magnitude of the optical companion decreased by 0.2 M in less than
  one year, in passbands U, B. and V. The infrared magnitude decreased by
  0.6 M in the K band and the ultraviolet flux is nearly invariable. The
  variations in different wavelength regions are probably due to changes
  in the circumstellar envelope. November 1981 high resolution IUE spectra
  clearly show C IV and Si IV lines with P Cygni profiles. February
  and October 1980 profiles did not show this characteristic (due to
  intrinsic variability of the source and/or a consequence of the smaller
  S/N ratio of the spectra). From the Si IV and C IV P Cygni profiles,
  a mass loss rate of 6 X 10 to the minus 9th to 10 to the minus 8th
  power M/yr is estimated. From the infrared excess, a mass loss rate
  of 6 x 10 to the minus 6th power M/yr is obtained. Radio observations
  at 18 cm give an upper limit of 36 mJy from A 0535+26.

---------------------------------------------------------
Title: Be components in X-ray binaries
Authors: De Loore, C.; Burger, M.; Mouchet, M.; van Dessel, E. L.
1982IAUS...98..347D    Altcode:
  The parameters of Be X-ray binaries, the most important spectral lines
  of three such sources, and the evolutionary tracks and positions of Be
  components are discussed. It is found necessary to study the variability
  of the entire spectral range, from X-rays to IR, in order to determine
  whether Be X-ray sources are binaries. Although an optical orbit has
  not yet been derived for any of the sources in question, two arguments
  are adduced on behalf of their binary character: the fact that the
  X-ray pulsation is the signature of a rotating compact object, and
  the determination that several classical Be stars are binaries. Such
  systems could be precursors for Be X-ray systems.

---------------------------------------------------------
Title: Mass Determination of Massive X-Ray Binaries
Authors: De Loore, C.; Mouchet, M.; van Dessel, E. L.; Burger, M.
1982Msngr..27...14D    Altcode:
  Massive X-ray binaries consist of anormal component of spectral type 0
  or B which is transferring matter to a compact companion, generally a
  neutron star, with possibly one exception, Cyg X-1, where the compact
  component could be a black hole. These compact stars have enormous
  magnetic fields (of the order of 1012 gauss), and extremely large
  gravities; accreted matter will be accelerated to velocities of half
  the light velocity, and guided by the field lines to restricted areas
  near the magnetic poles, the hot spots. These regions acquire in this
  way temperatures of the order of 107 K, and X-rays are generated. The
  X-rays are transported outwards as beams, and since the compact objects
  rotate rapidly, X-rays are observed as pulse-shaped beams.

---------------------------------------------------------
Title: Ultraviolet observations of the Be star and X-ray binary 4U
    1145-61 (=HD 102567 = HEN 715) obtained with the IUE.
Authors: De Loore, C.; Burger, M.; Hensberge, H.; van Dessel, E. L.
1981A&A...104..150D    Altcode:
  Two high resolution spectrograms in the range of 1150-2050 A were
  obtained by the IUE satellite, and from the spectrograms line lists
  of the stellar and interstellar absorption were compiled. The most
  important ions were found to be He (+); one, two and three times ionized
  C and Si; two and three times ionized O, three times ionized Mn; and
  two, three and four times ionized N. Eight interstellar molecular bands
  of (C-12)(O-16) of the fourth positive system were found, although
  the (C-13(O-16) bands were not detected. Due to uncertainties and
  the observed ionization fractions in other early-type stars, it is
  concluded that the mass loss rate of HD 102567 is between 10 to the
  -9th and 10 to the -10th solar mass/yr, with a most probable value of
  3 x 10 to the -10th solar mass/yr.

---------------------------------------------------------
Title: IUE and optical observations of V861 Sco.
Authors: Howarth, I. D.; Wilson, R.; Carter, B. S.; Menzies, J. W.;
   Roberts, G.; Whitelock, P. A.; van Dessel, E. L.; De Loore, C.;
   Sanford, M. C. W.; Burger, M.
1981A&A....93..219H    Altcode:
  We present the first results of high dispersion (Δλ ≃ 0.2 Å)
  IUE spectra of the possible X-ray binary V 861 Sco (HD 152667) taken
  at several orbital phases. Contemporary optical spectroscopy, uvbyβ
  and infrared photometry are also reported. <P />The UV spectrum is
  quite normal for the spectral type (B0Ia), with P Cygni profiles
  on a number of lines. Several of these lines show sharp multiple
  absorption components. The high ionisation interstellar species are not
  significantly enhanced by possible Xray emission. There are no large
  phase dependent variations in the UV spectra available; the optical
  spectra show significant changes, particularly at Hα, which is seen
  in absorption and emission at different times. <P />Our photometry
  confirms earlier results in general. The IR data do not support an
  earlier suggestion of a non-stellar secondary; indeed, our data lend
  no support to the hypothesis of a compact companion. The mass loss
  rate is found to be 1 10<SUP>-5</SUP> M<SUB>sun</SUB> yr<SUP>-1</SUP>.

---------------------------------------------------------
Title: Data Inferred from Visual Binaries
Authors: van Dessel, E. L.; Dommanget, J.
1980IrAJ...14..226V    Altcode:
  A star can be identified as a binary by observing the separation between
  the components or their common proper motion, or by taking micrometer
  measurements. Orbital parameters are known through interferometry and
  statistical material on binaries provides evidence for theories on star
  formation. Different populations of binaries exist that vary in their
  orbital period, indicating that different formation processes are at
  work. Where the assumed Jeans mass nearly equals the total mass of
  the system, a single nucleus will be surrounded by matter organizing
  itself into one or more companions or into planets. Examination of the
  mass ratio of binary systems is biased toward detection of equal mass
  systems, but additional data may correct this. A discontinuity appears
  to exist between stellar/stellar and stellar/planetary mass ratios,
  but this must be regarded with much caution because of the increasing
  difficulty of observing the variability of radial velocity.

---------------------------------------------------------
Title: Simultaneous ultraviolet, optical and X-ray observations of
    the X-raysource Vel X-1 (HD 77581).
Authors: Dupree, A. K.; Gursky, H.; Black, J. H.; Davis, R. J.;
   Hartmann, L.; Matilsky, T.; Raymond, J. C.; Hammerschlag-Hensberge, G.;
   van den Heuvel, E. P. J.; Burger, M.; Lamers, H. J. G. L. M.; Vanden
   Bout, P. A.; Morton, D. C.; De Loore, C.; van Dessel, E. L.; Menzies,
   J. W.; Whitelock, P. A.; Watson, M.; Sanford, P. W.; Pollard, G. S. G.
1980ApJ...238..969D    Altcode:
  UV spectra (obtained by the IUE) of HD 77581, associated with the binary
  X-ray source Vela X-1, show a spectrum typical of an early B-type
  supergiant. However, the P Cygni profiles of strong resonance lines
  show substantial variations with orbital phase. These variations can be
  ascribed to the changing ionization state in the stellar wind caused by
  the X-ray emitting companion. X-ray and spectroscopic and photometric
  optical observations, simultaneous with the IUE observations, indicate
  behavior consistent with previous epochs.

---------------------------------------------------------
Title: IUE observations of the Be stars HD 102567 (4U 1145-61),
    X Per and GAM Cas.
Authors: Hammerschlag-Hensberge, G.; van den Heuvel, E. P. J.; Lamers,
   H. J. G. L. M.; Burger, M.; de Loore, C.; Glencross, W.; Howarth, I.;
   Willis, A. J.; Wilson, R.; Menzies, J.; Whitelock, P. A.; van Dessel,
   E. L.; Sanford, P.
1980A&A....85..119H    Altcode:
  The first analysis of ultraviolet spectroscopic observation obtained
  with the IUE satellite of the Be stars HD 102567, X Per, and Gamma
  Cas, which all are associated with X-ray sources, is presented. The
  ultraviolet data for HD 102567 (4U 1145-61) consist of low-resolution
  spectra covering the wavelength range 1150-3200 A. The ultraviolet
  fluxes are consistent with a reddening of the source of E(B-V)=0.45
  magnitude. For this source a complementary program of visible photometry
  and spectroscopy and X-ray photometry was carried out. During the IUE
  observations the source 4U 1145-61 was not detectable in X-rays while
  the spectroscopic observations show dramatic intensity variations of
  the lower Balmer lines. For the bright Be stars Gamma Cas and X Per
  high-resolution (0.2 A) ultraviolet spectra covering the wavelength
  range 1150-3200 A have been obtained. The asymmetric profiles of
  resonance lines which are present in the spectra of both Gamma Cas
  and X Per indicate mass loss rates of 7 x 10 to the -9th and 10 to
  the -8th solar masses/yr, respectively.

---------------------------------------------------------
Title: Simultaneous observations of V861 Sco.
Authors: De Loore, C.; Burger, M.; Howarth, I. D.; Wilson, R.; Carter,
   B. S.; Menzies, J. W.; Roberts, G.; Whitelock, P. A.; van Dessel,
   E. L.; Sandford, M. C. W.
1980ESASP.157..237D    Altcode: 1980IUE2n......237D; 1980iue..conf..237D
  High dispersion spectra of V861 Sco (HD 152667) taken with International
  Ultraviolet Explorer at several orbital phases are presented, as
  well as simultaneous optical spectroscopy, and UVBY and infrared
  photometry. The UV spectrum is normal for a BOIa supergiant; a number
  of lines show P Cygni profiles with, in several cases, sharp multiple
  absorption components. No large phase dependent variations in the UV
  are detectable. The optical spectra reveal significant changes at H, He
  I 6678 and especially at H which is seen in emission and in absorption
  at different times. The velocity variability is strongly correlated
  with the outward velocity in the sense that velocities further out
  in the wind show more variability. The infrared photometry does not
  support the idea of a compact secondary. An evolutionary scenario,
  starting from a ZAMS-system of 80 solar masses + 10 solar masses is
  developed leading to an actual system of a 34 solar masses (BOI a)
  primary with a 10 solar mass (B2V) companion. The primary which just
  ignited helium in the core is nearly filling its Roche lobe, and will
  start soon (or has just started) a case B of mass transfer. The mass
  loss rate is estimated from the UV at 1.5 x 10 to the minus 6th power
  solar masses/year, and from theoretical considerations of the system
  parameters at 2.5 x 10 to the minus 6th power solar masses/year infrared
  excess points to 0.00005 solar masses/year.

---------------------------------------------------------
Title: Ultraviolet, visible, infrared and X-ray observations of
    SCO X-1.
Authors: Willis, A. J.; Wilson, R.; vanden Bout, P.; Sanner, F.;
   Black, J.; Davis, R. J.; Dupree, A. K.; Gursky, H.; Hartmann, L.;
   Raymond, J.; Matilsky, T.; Burger, M.; De Loore, C.; van Dessel,
   E. L.; Whitelock, P.; Menzies, J.; Meikle, W. P. S.; Joseph, R. D.;
   Sanford, P.; Pollard, G.; Sandford, M. C. W.
1980ApJ...237..596W    Altcode:
  The first UV spectroscopic observations of the X-ray source Scorpius
  X-1, obtained with the IUE satellite, are presented. The UV data
  consist of low-resolution spectra in the 1150-3200 A wavelength range,
  and show emission lines arising in Si II and IV; C III and IV; N III,
  IV, and V; O IV and V, and He II. Also discussed are observations
  using visible photometry and spectroscopy, and infrared and X-ray
  photometry. Significant changes between the strengths of the emission
  lines with phase are observed when the source changes its UV and
  optical brightness. Significant variations are also observed in the
  UV continuum brightness of Sco X-1 which approximately match those
  observed simultaneously in the visible B band. The color excess of
  Sco X-1 is found to be 0.35 plus or minus 0.05, and the UV continuum
  energy distribution is shown to be well fitted by a bremsstrahlung
  distribution.

---------------------------------------------------------
Title: Photometric observations of X Persei made in January -
    February 1979 with the one meter-telescope at Gornergrat.
Authors: van Dessel, E. L.
1980BAORB...9..159V    Altcode:
  No abstract at ADS

---------------------------------------------------------
Title: De IUE röntgenveertiendaagse.
Authors: Burger, M.; van Dessel, E. L.; De Loore, C.; Willis, A. J.
1980Zenit...7..218B    Altcode:
  No abstract at ADS

---------------------------------------------------------
Title: Het eerste jaar van IUE.
Authors: Willis, A. J.; De Loore, C.; van Dessel, E. L.; Burger, M.
1980Zenit...7..138W    Altcode:
  No abstract at ADS

---------------------------------------------------------
Title: Observations of X Persei in the U B2 V1 Colours of the
    Geneva System
Authors: van Dessel, E. L.; Burger, M.; de Loore, C.; Packet, W.;
   Vanbeveren, D.
1979IBVS.1679....1V    Altcode:
  No abstract at ADS

---------------------------------------------------------
Title: Radial Velocities of Visual Binaries
Authors: van Dessel, E. L.
1979Msngr..18....1V    Altcode:
  In addition to the initial chemical composition, the mass of a star is
  a fundamental parameter; it determines the life of the star from its
  birth, through its long or short period of luminous glory and to its
  inevitable end as a compact object. And yet, few stars have actually
  had their mass accurately measured. The programme that has recently
  been undertaken by Dr. Edwin van Dessel of the Royal Observatory in
  Brussels, Belgium, is therefore of particular importance. By obtaining
  precise measurements of radial velocities of stars in double or multiple
  systems, Dr. van Dessel expects soon to add new, welldetermined stellar
  masses to the present, all to short list.

---------------------------------------------------------
Title: Non-conservative evolution of massive close binaries including
    stellar wind mass loss.
Authors: Vanbeveren, D.; de Grève, J. P.; van Dessel, E. L.; de
   Loore, C.
1979A&A....73...19V    Altcode:
  No abstract at ADS

---------------------------------------------------------
Title: Conservative and non-conservative evolutionary computations
    in connection with Wolf-Rayet binaries.
Authors: Vanbeveren, D.; De Greve, J. P.; De Loore, C.; van Dessel,
   E. L.
1979IAUS...83..483V    Altcode:
  No abstract at ADS

---------------------------------------------------------
Title: The influence of stellar wind mass loss on the evolution of
    massive close binaries
Authors: Vanbeveren, D.; De Greve, J. P.; De Loore, C.; van Dessel,
   E. L.
1979IAUS...83..409V    Altcode:
  No abstract at ADS

---------------------------------------------------------
Title: IUE ultraviolet and complementary visible and X-ray
    observations of SCO X-1
Authors: Willis, A. J.; Wilson, R.; vanden Bout, P.; Sanner, F.;
   Black, J.; Davis, R. J.; Dupree, A. K.; Gursky, H.; Hartmann, L.;
   Matilsky, T.; Burger, M.; De Loore, C.; van Dessel, E. L.; Whitelock,
   P.; Menzies, J.; Sanford, P.; Pollard, G.; Sandford, M. C. W.
1979IUE1.symp..291W    Altcode:
  IUE observations providing the first ultraviolet spectroscopic data
  of the X-ray source Sco X-1 are presented and discussed. The IUE data
  were obtained in the low resolution mode and cover the wavelength range
  1150-3200 A. Data were obtained at many different phases and cycles
  in the binary period of the system of 0d.8. The short wavelength IUE
  spectra are dominated by numerous emission lines in Si II, IV, C III,
  IV, N III, IV, V, O IV, V and He II. The variations in the strengths
  of these lines both as a function of binary phase and brightness level
  of the source is discussed as well as those observed in the visible
  spectra of the source. The observed line strength variations can
  be explained in terms of a varying level of ionization with varying
  ionising X-ray radiation emitted from the compact object.

---------------------------------------------------------
Title: Radial velocities of visual binaries with an orbit derived
    from astrometric observations. II
Authors: van Dessel, E.
1979MRASB..41....1V    Altcode: 1979STIA...8021990V
  The list of visual binaries compiled by van Dessel (1977), for which
  an orbit had been computed from astrometric observations and which are
  believed to be capable of yielding useful radial velocity determinations
  in the near future, is updated and extended. Three kinds of systems
  are included in the updated list: (1) binaries of which at least one
  component has been shown to be spectroscopically double (triple and
  multiple systems); (2) binaries that are suspected of containing
  a third component because of the large scatter in radial velocity
  values; and (3) binaries for which the semiamplitude of the relative
  radial velocity variation is greater than 15 km/sec, according to the
  computed orbital elements.

---------------------------------------------------------
Title: Orbit of the visual binary ADS 3588 = IDS 04546 S 1632.
Authors: van Dessel, E.
1978BAORB...9...44V    Altcode:
  No abstract at ADS

---------------------------------------------------------
Title: The Evolution of Massive Close Binaries, VI: Final
    Considerations for the Conservative Case
Authors: De Greve, J. P.; De Loore, C.; van Dessel, E. L.
1978Ap&SS..53..105D    Altcode:
  The results of evolutionary computations for massive binary systems
  (initial masses of the primary ≳10M <SUB>⊙</SUB>) with mass ratios
  between 0.3 and 0.8 are summarized and compared with observations in
  order to verify how far one can go with the conservative assumption
  of mass exchange. It is found that conservative mass exchange
  leads to acceptable first-order models of W-R and massive X-ray
  binaries. However, the comparison between this theory and observation
  reveals that for the observed systems (W-R and X-ray binaries) a
  preference exists for low intial mass ratios; moreover, the X-ray
  luminosities of the theoretical models are systematically too low,
  though this may be due to the adopted wind model. In addition, the
  influences of several parameters (distance between the components,
  chemical composition, primary mass, mass ratio and atmosphere) are
  examined. These parameters influence the remnant mass and any further
  evolution only marginally. Attention is also given to the effect
  on the system parameters of a supernova explosion of the remnant of
  the mass-losing component. For a large range of systems a disruption
  probability smaller than 25% is found.

---------------------------------------------------------
Title: Occultations d'étoiles par la lune, observées à
    l'équatorial de 45 cm de 1974 à 1977.
Authors: Dommanget, J.; van Dessel, E.
1978BAORB...9...32D    Altcode:
  No abstract at ADS

---------------------------------------------------------
Title: Spectroscopic observers please help!
Authors: van Dessel, E. L.
1977Obs....97..203V    Altcode:
  No abstract at ADS

---------------------------------------------------------
Title: Radial velocities of visual binaries with an orbit derived
    from astrometric observations.
Authors: van Dessel, E.
1977tras.conf..151V    Altcode:
  No abstract at ADS

---------------------------------------------------------
Title: Orbital elements and removal of the nodal ambiguity for the
    visual binary ADS 7390 = ω Leo
Authors: van Dessel, E. L.
1976A&AS...26..415V    Altcode:
  Orbital elements and ephemeris of the binary ADS 7390. The ascending
  node is identified on the basis of high resolution spectra. Key words:
  visual binaries - orbit - radial velocities

---------------------------------------------------------
Title: Radial velocities of the visual binary 70 Ophiuchi.
Authors: Batten, A. H.; van Dessel, E. L.
1976PDAO...14..345B    Altcode:
  No abstract at ADS

---------------------------------------------------------
Title: Dubbelsterren (2) - (4). Meervoudige sterren eerder regel
    dan uitzondering.
Authors: van Dessel, E. L.
1976Zenit...3...20V    Altcode:
  No abstract at ADS

---------------------------------------------------------
Title: Observation photographique de l'éclipse de Soleil du 29
    avril 1976 à l'équatorial Cooke-Zeiss.
Authors: Dommanget, J.; van Dessel, E.; Nys, O.
1976BAORB...8..325D    Altcode:
  No abstract at ADS

---------------------------------------------------------
Title: Line Intensities in the Photosphere-Chromosphere Transition
Region. IV: Cr I and Metallic Ion Lines
Authors: van Dessel, E. L.
1975SoPh...44...13V    Altcode:
  Eclipse observations of total line intensities (Cr I: two groups of
  lines; Ti II, Fe II and Cr II: two lines each) are interpreted in
  terms of departures from LTE. The same method as described in Paper
  III (van Dessel, 1974) is used. The HSRA model is used to compute
  the LTE populations. A distribution of NLTE-coefficients is obtained
  for each group of lines. The lines discussed in the present paper are
  seen to remain in emission down to some 1000 km inside the limb. As
  a consequence, interpretation is less simple than for the Fe I lines
  (Paper III); population and excitation temperatures are found to be
  rather divergent from Holweger's temperature, which was used for a
  first approximation.

---------------------------------------------------------
Title: Dubbelsterren (1). Indeling gebaseerd op waarnemingsmethoden.
Authors: van Dessel, E. L.
1975Zenit...2..419V    Altcode:
  No abstract at ADS

---------------------------------------------------------
Title: Line Intensities in the Photosphere-Chromosphere Transition
Region. III: Empirical NLTE Analysis of FeI Lines
Authors: van Dessel, E. L.
1974SoPh...38..351V    Altcode:
  We analyse Fe I lines observed during the 1961 eclipse at Brač,
  Yugoslavia (see paper II: van Dessel et al., 1973), using a computer
  program for the calculation of theoretical line intensities, which
  was described in Paper I (van Dessel, 1970). A few minor modifications
  to the physical input are discussed in Section 2. NLTE-coefficients,
  affecting the line absorption coefficient and the source function,
  are introduced and discussed in Section 3. Starting from coefficients
  derived from the combination T<SUB>el</SUB> (HSRA) + T<SUB>ex</SUB>
  (Holweger), suitable distributions with height of the NLTE-coefficients
  are determined for the most striking cases among the observed
  lines. Only little deviation from the populations derived from
  Holweger's temperature distribution is needed to explain the observed
  line behaviour.

---------------------------------------------------------
Title: Occultations d'étoiles par la lune, observées à
    l'équatorial de 45 cm en 1972 et 1973.
Authors: Dommanget, J.; van Dessel, E.
1974BAORB...8..141D    Altcode:
  No abstract at ADS

---------------------------------------------------------
Title: Line-Intensities in the Photosphere-Chromosphere Transition
Region. II: Observational Material from the 1961 Eclipse at Brač
Authors: Van Dessel, E. L.; Houtgast, J.; Koelbloed, D.
1973SoPh...33..375V    Altcode:
  We present results from eclipse spectra in the wavelength region
  4588-4682 Å, taken during the eclipse of February 15, 1961 at Brač,
  Yugoslavia. Absolute line intensities have been determined in the
  photosphere-chromosphere transition region. The method of reduction is
  discussed in Section 2 and the observed variation of the total intensity
  as a function of the height is shown for a number of lines in Figures
  5-8. The results for the Fe I lines are compared with computations
  (as described in Paper I: van Dessel, 1970) for various solar model
  atmospheres (Section 4). The model, which combines Holweger's (1967)
  temperature distribution for the excitation temperature with the HSRA
  model (Gingerich et al., 1971) for the electron temperature, yields
  a better agreement than all pure LTE-models.

---------------------------------------------------------
Title: New orbit and mass of the visual binary and magnetic Ap star
    ADS 7334 = HR 3724.
Authors: van Dessel, E. L.
1972A&A....21..155V    Altcode:
  Summary. Calculation of the orbital elements, physical characteristics
  and ephemeris of the visual binary ADS 7334. A previous orbit of this
  star, computed by Finsen (1968), is shown to be unsatisfactory. The
  present orbit is in better agreement with spectroscopic observations by
  van den Heuvel (1971) and leads to plausible masses. Resumee'. Calcul
  des e'le'ments orbitaux, des elements physiques et de l'e'phe'me'nde
  du couple ADS 7334. On montre qu'une orbite antefleure, calculee par
  Finsen (1968) pour cette etoile, ne donne pas satisfaction. L'orbite
  actuelle est en meilleur accord avec les observations spectroscopiques
  de van den Heuvel (1971) et conduit a' des masses plausibles. Key words:
  orbital elements - visual binary - peculiar A stars - magnetic stars

---------------------------------------------------------
Title: Occultations d'étoiles par la lune observées à l'équatorial
    de 45 cm, en 1969, 1970 et 1071.
Authors: Dommanget, J.; van Dessel, E.
1972BAORB...8...42D    Altcode:
  No abstract at ADS

---------------------------------------------------------
Title: Passage de Mercure sur le disque solaire le 9 mai
    1970. Observations photographiques à l'équatorial Cooke-Zeiss.
Authors: Dommanget, J.; van Dessel, E.; Nys, O.
1971BAORB...7..188D    Altcode:
  No abstract at ADS

---------------------------------------------------------
Title: A Comparison of Computed and Observed Line Profiles and Flash
    Intensities in the Photosphere-Chromosphere Transition Region
Authors: Van Dessel, E. L. J.
1970SoPh...15..322V    Altcode:
  This paper mainly deals with the development of a method for the
  interpretation of eclipse observations in the extreme limb - lower
  chromosphere transition region. We compute line profiles emitted by a
  column of 1 cm<SUP>2</SUP> cross section along the line of sight and,
  by integration, profiles and total (flash) intensities from a slice
  of 1 cm width beyond the Moon's edge, at various heights with respect
  to the solar limb. The solar models used are mentioned in Section 1;
  method and approximations are described in Section 2. Calculations have
  been made for some FeI lines with various equivalent widths (Table I);
  the results are discussed in Section 3. It appears that the method
  enables one to distinguish between the various models. Particularly
  line intensities just inside the limb are very important.

---------------------------------------------------------
Title: Preliminary orbit of the visual binary ADS 9975 = A 1642 =
    JDS 2417.
Authors: Dommanget, J.; van Dessel, E. L.
1970A&A.....6..423D    Altcode:
  Calculation of the orbital elements and physical characteristics of
  the visual binary ADS 9975, adopting a change of quadrant for the
  observations later than 1950. This assumption is based on the possible
  variability of one of the components. Calcul des e'ments orbitaux et
  des 6ments physiques du couple ADS 9975, dans l' d'un changement de
  quadrant intervenu aux environs de 1950. Cette est sur une variabilit6
  d'6datpossible de l'une des composantes. Key words: orbital elements -
  visual binary