Light curves of the triple system V906 Sco (Vaz+ 1997)

Details Light curves of the triple system V906 Sco (Vaz+ 1997) Light curves of the triple system V906 Sco (Vaz+ 1997)

Apr 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ycat..41250471v&link_type=abstract

VizieR On-line Data Catalog: J/A+AS/125/471. Originally published in: 1997A&AS..125..471V

Computer Science

Binaries: Eclipsing, Photometry: Uvby

Scientific paper

Complete uvby light curves of the detached triple-lined late B-type eclipsing binary V906 Scorpii, obtained from 1987 to 1991, are presented. A detailed photometric analysis based on these observations and on new spectroscopic material yields accurate masses and radii (errors <2%) for the components, confirms that the system is member of NGC 6475 (Messier 7) and is published separately (Alencar et al., 1997A&A...326..709A) (1 data file).

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