Radial Velocity Studies of Southern Close Binary Stars. II. Spring/Summer Systems*

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Published 2006 December 7 © 2007. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Hilmar W. Duerbeck and Slavek M. Rucinski 2007 AJ 133 169 DOI 10.1086/509764

1538-3881/133/1/169

Abstract

Radial velocity measurements and sine-curve fits to the orbital velocity variations are presented for 14 close binary stars, S Ant, TT Cet, TW Cet, AA Cet, RW Dor, UX Eri, YY Eri, BV Eri, CT Eri, SZ Hor, AD Phe, TY Pup, HI Pup, and TZ Pyx. All are double-lined binaries, and all except the last one are contact binaries. The orbital data must be considered preliminary because of the relatively small number of observations (6-12), a circumstance that is partly compensated by the good definition of the broadening functions used for the radial velocity determinations.

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Footnotes

  • Based on data obtained at the European Southern Observatory.

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10.1086/509764