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The Apsidal Motion of the Eclipsing Binary Systems GSC 4487 0347 and GSC 4513 2537

Published online by Cambridge University Press:  23 April 2012

V. S. Kozyreva ,
A. V. Kusakin ,
T. Krajci ,
J. Menke  and
T. M. Tsvetkova
V. S. Kozyreva
Affiliation:
Sternberg State Astronomical Institute, 13, University avenue, 119992, Moscow, Russia, email: [email protected]
A. V. Kusakin
Affiliation:
National space agency republic of Kazakhstan, JSCNCSRT Department “V.G. Fesenkov Astrophysical Institute”, 050068, Almaty, Kazakhstan
T. Krajci
Affiliation:
Astrokolkhoz Observatory, PO Box 1351, Cloudcroft, 88317, New Mexico, USA
J. Menke
Affiliation:
Starlight Farm Observatory, 22500 Old Hudred Rd, Barnesville, MD 20838, USA
T. M. Tsvetkova
Affiliation:
Institute of Astronomy Russian Academy of Sciences, 48 Pyatnitskaya st., 119017, Moscow, Russian
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Abstract

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The eclipsing variable stars GSC 44870347 and GSC 4513 2537 are recently discovered binary systems (Otero et al., 2006) with orbital periods 1d.99 and 6d.33 days. We carried out the photometric observations of these eclipsing binaries from 2009-2010 using a CCD-array at the Tien-Shan Observatory in Kazakstan, at the Crimea Station of the Sternberg Astronomical Institute, at the Astrokolkhoz Observatory in New Mexico (AAVSO), while the spectrophotometric observations were obtained at the Starlight Farm Observatory in Barnesville, USA.

Keywords

eclipsing binarymulticolour photometryapsidal motion
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S282: From Interacting Binaries to Exoplanets: Essential Modeling Tools , July 2011 , pp. 93 - 94
Copyright
Copyright © International Astronomical Union 2012

References

Otero, S. A., Wils, R., Hoogeveen, G., & Dubovsky, P. A. 2006, IBVS, 5681Google Scholar