Apsidal motion in eccentric eclipsing binary WW Camelopardalis

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dc.contributor.author Wolf, Marek
dc.contributor.author Kotková, Lenka
dc.contributor.author Kocián, R.
dc.contributor.author Dřevěný, R.
dc.contributor.author Hanžl, D.
dc.date.accessioned 2011-01-12T08:42:06Z
dc.date.available 2011-01-12T08:42:06Z
dc.date.issued 2010
dc.identifier.citation The astronomical journal. 2010, vol. 139, no. 3, p. 1028-1030. en
dc.identifier.issn 0004-6256
dc.identifier.issn 1538-3881
dc.identifier.uri http://hdl.handle.net/10084/83563
dc.description.abstract WW Camelopardalis is a relatively bright eclipsing binary system with a slightly eccentric orbit. A dozen of its new eclipse times were measured as part of our long-term observational project of eccentric eclipsing binaries. Based on a new solution of the current O – C diagram, we found for the first time an apsidal motion in good agreement with theory. Its period is about 370 ± 50 years. The determined internal structure constant is close to the theoretically expected value. The relativistic effect is significant, being about 13% of the total apsidal motion rate. en
dc.language.iso en en
dc.publisher IOP Publishing en
dc.relation.ispartofseries The astronomical journal en
dc.relation.uri http://dx.doi.org/10.1088/0004-6256/139/3/1028 en
dc.subject binaries: eclipsing en
dc.subject stars: fundamental parameters en
dc.subject stars: individual (WW Cam) en
dc.title Apsidal motion in eccentric eclipsing binary WW Camelopardalis en
dc.type article en
dc.identifier.location Není ve fondu ÚK en
dc.identifier.doi 10.1088/0004-6256/139/3/1028
dc.identifier.wos 000274429600018

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