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Eccentricity of Selected Eclipsing Systems

Published online by Cambridge University Press:  23 April 2012

W. Ogłoza ,
J. M. Kreiner ,
G. Stachowski ,
B. Zakrzewski ,
Z. Mikulášek  and
M. Zejda
W. Ogłoza
Affiliation:
Mt. Suhora Observatory, Cracow Pedagogical University, 30-084 Cracow, ul Podchorażych 2, Poland email: ogloza@up.krakow.pl
J. M. Kreiner
Affiliation:
Mt. Suhora Observatory, Cracow Pedagogical University, 30-084 Cracow, ul Podchorażych 2, Poland email: ogloza@up.krakow.pl
G. Stachowski
Affiliation:
Mt. Suhora Observatory, Cracow Pedagogical University, 30-084 Cracow, ul Podchorażych 2, Poland email: ogloza@up.krakow.pl
B. Zakrzewski
Affiliation:
Mt. Suhora Observatory, Cracow Pedagogical University, 30-084 Cracow, ul Podchorażych 2, Poland email: ogloza@up.krakow.pl
Z. Mikulášek
Affiliation:
Masaryk University, Brno, Czech Republic
M. Zejda
Affiliation:
Masaryk University, Brno, Czech Republic
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Abstract

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This paper presents the results of verification of known stars showing evidence of orbital eccentricity and apsidal motion.

Keywords

stars: binaries: eclipsingephemerides
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. 61 - 62
Copyright
Copyright © International Astronomical Union 2012

References

Kreiner, J. M. 2004, AcA, 50, 247Google Scholar