Free Access
Astron. Astrophys. Suppl. Ser.
Volume 140, Number 3, December II 1999
Page(s) 293 - 307
Published online 15 December 1999
DOI: 10.1051/aas:1999423

Astron. Astrophys. Suppl. Ser. 140, 293-307

A comparative study of the long-term light variations of six young irregular variables

J. Gürtler1 - C. Friedemann1 - H.-G. Reimann1 - E. Splittgerber2 - E. Rudolph3

Send offprint request: J. Gürtler

1 - Friedrich-Schiller-Universität Jena, Astrophysikalisches Institut und Universitäts-Sternwarte, Schillergäßchen 2, D-07745 Jena, Germany
2 - Ludwig-Stur-Straße 5, D-06108 Halle/Saale, Germany
3 - Lieselotte-Hermann-Straße 38a, D-07747 Jena, Germany

Received April 17, 1998; accepted September 13, 1999


We investigated the long-term light variations of six young irregular variables, all of them UX Orionis stars or related objects. For this aim we determined new photographic magnitudes for the five stars VX Cas, BH Cep, BO Cep, SV Cep, and RZ Psc and made use of similar data for WW Vul published independently. The magnitudes were derived from Argelander brightness estimates performed on plates of the Harvard College Observatory and Sonneberg Observatory plate collections. The data cover a period of about 100 years and are available at the Centre des Données Stellaires, Strasbourg. The new data were supplemented by multicolour photoelectric measurements taken from the literature and visual estimates collected by the AAVSO. The resulting lightcurves are displayed and discussed. Algol-like minima are observed with all the stars. Their properties are discussed under the presumption that they are caused by circumstellar dust clouds orbiting the stars. Parameters of the circumstellar dust shells are derived from modelling the observed infrared excess radiation and compared with constraints from the light variations.

Key words: stars: individual: VX Cas, BH Cep, BO Cep, SV Cep, RZ Psc, WW Vul -- stars: variables: general -- circumstellar matter

SIMBAD Objects

Copyright The European Southern Observatory (ESO)

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