Physical Parameters of Some Close Binaries: ET Boo, V1123 Tau, V1191 Cyg, V1073 Cyg and V357 Peg

Abstract

With the aim of providing new and up-to-date absolute parameters of some close binary systems, new BVR CCD photometry was carried out at the Ankara University Observatory (AUG) for five eclipsing binaries, ET Boo, V1123 Tau, V1191 Cyg, V1073 Cyg and V357 Peg between April, 2007 and October, 2008. In this paper, we present the orbital solutions for these systems obtained by simultaneous light and radial velocity curve analyses. Extensive orbital solution and absolute parameters for ET Boo system were given for the first time through this study. According to the analyses, ET Boo is a detached binary while the parameters of four remaining systems are consistent with the nature of contact binaries. The evolutionary status of the components of these systems are also discussed by referring to their absolute parameters found in this study.

this accepted paper will be published in New Astronomy

References in corpus (5)

• Contact Binaries with Additional Components.I. The Extant Data
• Contact binaries with additional components. III. The adaptive optics detections
• Radial Velocity Studies of Close Binary Stars. XI
• Radial Velocity Studies of Close Binary Stars.XIII
• Marginally low mass ratio close binary system V1191 Cyg

Cited by in corpus (6)

• Photometric study and absolute parameters estimation of six totally eclipsing contact binaries
• Investigation of the Orbital Period and Mass Relations for W UMa-type Contact Systems
• Starspots in contact and semi-detached binary systems
• Physical parameters of close binary systems: VIII
• Chromospheric activity in bright contact binary stars
• Photometric and spectroscopic studies of the long period low mass ratio deep contact binary KN Per