Radial Velocity Studies of Close Binary Stars.XIII

Details Radial Velocity Studies of Close Binary Stars.XIII Radial Velocity Studies of Close Binary Stars.XIII

2008-05-12

arxiv.org/abs/0805.1695v1

Astronomy and Astrophysics

Astrophysics

Accepted by AJ. 19 pages including 5 figures

Scientific paper

10.1088/0004-6256/136/2/586

Radial-velocity measurements and sine-curve fits to the orbital radial velocity variations are presented for ten close binary systems: EG Cep,V1191 Cyg, V1003 Her, BD+7_3142, V357 Peg, V407 Peg, V1123 Tau, V1128 Tau, HH UMa, and PY Vir. While most of the studied eclipsing systems are contact binaries, EG Cep is a detached or a semi-detached double-lined binary and V1003 Her is a close binary of an uncertain type seen at a very low inclination angle. We discovered two previously unknown triple systems, BD+7_3142 and PY Vir, both with late spectral-type (K2V) binaries. Of interest is the low-mass ratio (q = 0.106) close binary V1191 Cyg showing an extremely fast period increase; the system has a very short period for its spectral type and shows a W-type light curve, a feature rather unexpected for such a low mass-ratio system.

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