Four-colour photometry of eclipsing binaries .38. Light curves of the triple system V906 Scorpii

DOI: 
Publication date: 
01/11/1997
Main author: 
Vaz, LPR
IAA authors: 
Authors: 
Vaz, LPR; Andersen, J; Clausen, JV; Helt, BE; Garcia, JM; Gimenez, A; Alencar, SHP
Journal: 
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES
Publication type: 
Article
Volume: 
125
Pages: 
471-473
Number: 
Abstract: 
Complete uvby light curves of the detached triple-lined late B-type eclipsing binary V906 Scorpii, secured 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 less than or similar to 2%) for the components, confirms that the system is a member of NGC 6475 (Messier 7), and is published separately (Alencar et al. 1997).
Database: 
WOK
Keywords: 
stars, binaries, eclipsing; stars, individual, V906 Sco