Rapid apsidal motion in V381 Cassiopeiae

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dc.contributor.author Wolf, Marek
dc.contributor.author Šmelcer, Ladislav
dc.contributor.author Kučáková, H.
dc.contributor.author Hynek, Tomáš
dc.contributor.author Onderková, K.
dc.contributor.author Svoboda, P.
dc.contributor.author Chrastina, Marek
dc.date.accessioned 2011-01-12T08:05:53Z
dc.date.available 2011-01-12T08:05:53Z
dc.date.issued 2010
dc.identifier.citation New astronomy. 2010, vol. 15, issue 6, p. 530-532. en
dc.identifier.issn 1384-1076
dc.identifier.uri http://hdl.handle.net/10084/83559
dc.description.abstract V381 Cas is a relatively bright and early-type eclipsing binary system. Several new times of its eclipses were measured as part of our long-term observational project of eccentric eclipsing binaries. Based on a current O–C diagram solution, we found for the first time that its orbit is slightly eccentric (e = 0.025) and shows a very rapid apsidal advance with short period of about 20 years only. The relativistic and third body effects are negligible, being about 3% of the total apsidal motion rate. en
dc.language.iso en en
dc.publisher Elsevier en
dc.relation.ispartofseries New astronomy en
dc.relation.uri http://dx.doi.org/10.1016/j.newast.2009.12.011 en
dc.subject stars: binaries : eclipsing en
dc.subject stars: individual: V381 Cas en
dc.subject stars: fundamental parameters en
dc.title Rapid apsidal motion in V381 Cassiopeiae en
dc.type Article en
dc.identifier.location Není ve fondu ÚK en
dc.identifier.doi 10.1016/j.newast.2009.12.011
dc.identifier.wos 000277751400005

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