XXXVI. Light curves of the O7V+O9V system V 3903 Sagittarii
Departamento de Física, ICEx, UFMG, C.P. 702, 30161–970 Belo Horizonte, MG, Brazil
2 Department of Astronomy, University of Wisconsin, wadison, Wisconsin 53706, U.S.A.
3 Laboratorio de Astrofísica Espacial y Física Fundamental, INTA, Apdo. 50727, 28080 Madrid, Spain
4 Astronomical Observatory, NBIfAFG, Juliane Maries Vej 30, DK-2100 Copenhagen, Denmark
5 Departamento de Física, E.U.I.T. Industriales, UPM, Ronda de Valencia 3, E-28012 Madrid, Spain
6 Instituto de Astrofísica de Andalucía, Apdo. 3004, E-18080 Granada, Spain
7 Sterrewacht Leiden, Leiden University, Niels Bohrweg 2, 2333 CA Leiden, The Netherlands
8 Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, U.S.A.
Send offprint request to: L.P.P. Vaz at address 1
Accepted: 11 July 1997
Complete uvby light curves of the young detached double-lined massive O-type eclipsing binary V 3903 Sagittarii, obtained from 1989 to 1994, are presented. The observations were obtained at two different sites and a discussion of the characteristics of both data sets is included.
Key words: binaries: eclipsing: spectroscopic / stars: individual: V 3903 Sgr / stars: early-type
Based on observations done with the ZEISS 60 cm telescope at the Pico dos Dias Observatory (PDO), National Laboratory of Astrophysics, LNA–CNPq, Brasópolis, MG, Brazil, and with the Danish 50 cm Telescope (SAT) at the European Southern Observatory (ESO), La Silla, Chile.
The Tables 2, 3 and 4, presented in this paper will be only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (18.104.22.168) or via http://cdsweb.u-strasbg.fr/Abstract.html
© European Southern Observatory (ESO), 1998