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Astron. Astrophys. 319, 481-486 (1997) Red giants in open clustersVI. Orbits of ten spectroscopic binaries * **
J.-C. Mermilliod 1,
J. Andersen 2 and
M. Mayor 3
Received 11 July 1996 / Accepted 23 July 1996 Abstract We present new orbits for ten (single-lined) spectroscopic binaries
in seven open clusters: NGC 2489, 2567, 3033, 5822, 6134, 6664 and IC
2488 based on 243 individual radial velocities obtained with the
southern CORAVEL scanner. The orbital periods range from 98.5 to 3566
days. The shortest-period orbit is circular, as expected. Seven of the
binaries are confirmed cluster members, one is a possible member, and
two are clearly non-members. Maximum masses from photometric
separation and minimum masses from the spectroscopic orbits define the
mass of the secondaries within an interval of Key words: cluster:
open
* Based on observations collected with the Danish 1.54-m telescope at the European Southern Observatory, La Silla, Chile Send offprint requests to: J.-C. Mermilliod Contents
© European Southern Observatory (ESO) 1997 Online publication: July 3, 1998 ![]() |