Lpr. Vaz et al., 4-COLOR PHOTOMETRY OF ECLIPSING BINARIES .38. LIGHT CURVES OF THE TRIPLE SYSTEM V906-SCORPII, Astronomy & Astrophysics. Supplement series, 125(3), 1997, pp. 471-473
Complete uvby light curves of the detached triple-lined late B-type ec
lipsing binary V906 Scorpii, secured from 1987 to 1991, are presented.
A detailed photometric analysis based on these observations and on ne
w spectroscopic material yields accurate masses and radii (errors less
than or similar to 2%) for the components, confirms that the system i
s a member of NGC 6475 (Messier 7), and is published separately (Alenc
ar et al. 1997).