Four-colour photometry of eclipsing binaries. XXXVI. Light curves of the O7V+O9V system V 3903 Sagittarii

Details Four-colour photometry of eclipsing binaries. XXXVI. Light curves of the O7V+O9V system V 3903 Sagittarii Four-colour photometry of eclipsing binaries. XXXVI. Light curves of the O7V+O9V system V 3903 Sagittarii

Mar 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26as..128..251v&link_type=abstract

Astronomy and Astrophysics Supplement, v.128, p.251-254

Astronomy and Astrophysics

Astrophysics

1

Binaries: Eclipsing: Spectroscopic, Stars: Individual: V 3903 Sgr, Stars: Early-Type

Scientific paper

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. 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.

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