| dc.contributor.author | Wolf, Marek | |
| dc.contributor.author | Lehký, M. | |
| dc.contributor.author | Šmelcer, Ladislav | |
| dc.contributor.author | Kučáková, Hana | |
| dc.contributor.author | Kocián, Radek | |
| dc.date.accessioned | 2016-11-07T11:23:19Z | |
| dc.date.available | 2016-11-07T11:23:19Z | |
| dc.date.issued | 2011 | |
| dc.identifier.citation | New Astronomy. 2011, vol. 16, issue 6, p. 402-404. | cs |
| dc.identifier.issn | 1384-1076 | |
| dc.identifier.uri | http://hdl.handle.net/10084/116350 | |
| dc.description.abstract | Several new precise times of eclipses were measured for eclipsing binary CG Aur as a part of our long-term observational project for studying eclipsing binaries with an eccentric orbit. Based on a current O - C diagram, we found for the first time that its orbit is slightly eccentric (e = 0.124) and that times of minima besides the slow apsidal motion show very rapid changes with a period about 700 days only, caused very probably by the third body orbiting the eclipsing pair. The relativistic contribution to the total apsidal-motion rate is significant being about 33%. | cs |
| dc.language.iso | en | cs |
| dc.publisher | Elsevier | cs |
| dc.relation.ispartofseries | New Astronomy | cs |
| dc.relation.uri | http://dx.doi.org/10.1016/j.newast.2011.03.004 | cs |
| dc.rights | © 2011 Elsevier B.V. All rights reserved. | cs |
| dc.subject | stars: binaries: eclipsing | cs |
| dc.subject | stars: individual: CG Aur | cs |
| dc.subject | stars: fundamental parameters | cs |
| dc.title | The triple system CG Aurigae | cs |
| dc.type | article | cs |
| dc.identifier.doi | 10.1016/j.newast.2011.03.004 | |
| dc.type.status | Peer-reviewed | cs |
| dc.description.source | Web of Science | cs |
| dc.description.volume | 16 | cs |
| dc.description.issue | 6 | cs |
| dc.description.lastpage | 404 | cs |
| dc.description.firstpage | 402 | cs |
| dc.identifier.wos | 000290199700005 | |