A&A Supplement series, Vol. 128, March I 1998, 251-254
Received May 22; accepted July 11, 1997
Four-colour photometry of eclipsing binaries
L.P.R. Vaz, N.C.S. Cunha, J. Andersen, J.V. Clausen, J.M. Garcia, A. Giménez, B.W. Casey, and S. de Koff
Send offprint request: L.P.P. Vaz at address 1
Departamento de Fisica, ICEx, UFMG, C.P. 702, 30161-970 Belo Horizonte, MG, Brazil
Laboratorio de Astrofisica Espacial y Fisica Fundamental, INTA, Apdo. 50727, 28080 Madrid, Spain
Astronomical Observatory, NBIfAFG, Juliane Maries Vej 30, DK-2100 Copenhagen, Denmark
Departamento de Fisica, E.U.I.T. Industriales, UPM, Ronda de Valencia 3, E-28012 Madrid, Spain
Instituto de Astrofisica de Andalucıa, Apdo. 3004, E-18080 Granada, Spain
Department of Astronomy, University of Wisconsin, wadison, Wisconsin 53706, U.S.A.
Sterrewacht Leiden, Leiden University, Niels Bohrweg 2, 2333 CA Leiden, The Netherlands
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, U.S.A.
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.
keywords: binaries: eclipsing: spectroscopic -- stars: individual: V 3903 Sgr -- stars: early-typeSIMBAD Objects
Tables at the CDS
Copyright by the European Southern Observatory (ESO)