Radial Velocity Studies of Close Binary Stars.II

Abstract

Radial velocity measurements and simple sine-curve fits to the orbital velocity variations are presented for the second set of ten contact binary systems. Eight systems are of the A-type: AH Aur, CK Boo, DK Cyg, UZ Leo, XZ Leo, V839 Oph, GR Vir and NN Vir. V842 Her is the only W-type, while SV Equ appears to be a semi-detached system seen at a low orbital inclination rather than a contact binary. Several of the studied system are prime candidates for complete light and radial-velocity synthesis solutions.

Second paper of the series started with astro-ph/9902168. AASTeX. 2 tables, 3 figures

References in corpus (1)

• Radial Velocity Studies of Close Binary Stars.I

Cited by in corpus (26)

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• Radial Velocity Studies of Close Binary Stars.IV
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• Physical parameters of 62 eclipsing binary stars using the ASAS-3 data$-$I
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• Radial Velocity Studies of Close Binary Stars.V
• Radial Velocity Studies of Close Binary Stars.VI
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• Radial Velocity Studies of Close Binary Stars.VIII
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• Radial Velocity Studies of Close Binary Stars. XI
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• Radial Velocity Studies of Close Binary Stars. IX
• Radial Velocity Studies of Close Binary Stars.X
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• Radial Velocity Studies of Southern Close Binary Stars.I
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