Volume 465, Number 2, April II 2007
|Page(s)||549 - 556|
|Section||Stellar structure and evolution|
|Published online||05 February 2007|
A procedure for the classification of eclipsing binaries
Institute of Astronomy of the Russian Academy Sci. 48 Pyatnitskaya St., 119017 Moscow, Russia e-mail: firstname.lastname@example.org
2 Department of Physics, Moscow State University, 119992 Moscow, Russia
3 UMR 6091, Observatoire de Besançon – CNRS, 41bis avenue de l'Observatoire, 25010 Besançon Cedex, France
4 South African Astronomical Observatory, PO Box 9, Observatory 7935, South Africa
5 Department of Physics, Ural State University, Lenin Street 51, 620083 Ekaterinburg, Russia
6 Departament d'Astronomia i Meteorologia, Universitat de Barcelona, Avda. Diagonal 647, 08028 Barcelona, Spain
Accepted: 12 January 2007
A procedure for the automatic classification of eclipsing binaries is presented. The procedure is based on the data from 1029 classified systems and allows for the classification of a given system based on a set of observational parameters, even if the set is incomplete. The procedure is applied to six large surveys of eclipsing variables. About 5300 systems were classified for the first time and can be used for the determination of the astrophysical parameters of their components.
Key words: binaries: eclipsing / methods: data analysis / methods: statistical
© ESO, 2007
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