Astron. Astrophys. Suppl. Ser. 136, 419-420
D. Pourbaix1 and H. Eichhorn2
Send offprint request: D. Pourbaix,
e-mail: pourbaix@astro.ulb.ac.be
1 - Institut d'Astronomie et d'Astrophysique, Université Libre de
Bruxelles, C.P. 226, Boulevard du Triomphe, B-1050 Bruxelles, Belgium
2 -
Institut für Astronomie, University of Vienna, Austria
Received October 07; accepted December 01, 1998
Using a sample of binaries which were observed visually (VB) as well as spectroscopically for both components (SB2), we show that the efficiency almost always increases when a combined VB-SB2 solution replaces one based only on VB.
Key words: methods: numerical; statistical -- binaries: visual; spectroscopic
Copyright The European Southern Observatory (ESO)