IAA authors:
Clausen, J. V.;Helt, B. E.
Authors:
Vaz, L. P. R.;Andersen, J.;Clausen, J. V.;Helt, B. E.;Garcia, J. M.;Gimenez, A.;Alencar, S. H. P.
Journal:
Astronomy and Astrophysics Supplement Series
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 〈~ 2%) for the components, confirms that the system is a member of NGC 6475 (Messier 7), and is published separately \cite[(Alencar et al. 1997)]{ale97}. Based on observations done with the Danish 50 cm Telescope (SAT) at the European Southern Observatory (ESO), La Silla, Chile. Table 2 presented in this paper will only be accessible in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/Abstract.html
URL:
https://ui.adsabs.harvard.edu/#abs/1997A&AS..125..471V/abstract
Keywords:
STARS: BINARIES: ECLIPSING;STARS: INDIVIDUAL: V906 SCO