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dc.contributor.authorWolf, Marek
dc.contributor.authorHarmanec, Petr
dc.contributor.authorSarounová, Lenka
dc.contributor.authorZejda, Miloslav
dc.contributor.authorBožić, Hrvoje
dc.contributor.authorHornoch, Kamil
dc.contributor.authorKozyreva, V. S.
dc.contributor.authorHynek, Tomáš
dc.contributor.authorKrál, Lukáš
dc.date.accessioned2006-10-16T08:36:04Z
dc.date.available2006-10-16T08:36:04Z
dc.date.issued2004
dc.identifier.citationAstronomy and astrophysics. 2004, vol. 420, issue 2, p. 619-624.en
dc.identifier.issn0004-6361
dc.identifier.issn1432-0746
dc.identifier.urihttp://hdl.handle.net/10084/57129
dc.language.isoenen
dc.publisherEDP Sciencesen
dc.relation.ispartofseriesAstronomy and astrophysicsen
dc.relation.urihttp://dx.doi.org/10.1051/0004-6361:20035927en
dc.titleApsidal motion in eccentric eclipsing binaries: V871 Aql, V345 Lac, V401 Lac and CR Scten
dc.typearticleen
dc.identifier.locationNení ve fondu ÚKen
dc.description.abstract-enAbout thirty new times of minimum light recorded with photoelectric or CCD photometers were obtained for several little studied eccentric-orbit eclipsing binaries V871 Aql (P = 3(d).0, e = 0.13), V345 Lac (7(d).5, 0.46), V401 Lac (2(d).0, 0.10) and CR Sct (4(d).2, 0.09). Their O-C diagrams were analyzed using all reliable timings found in the literature and in all cases an apsidal motion was either discovered or confirmed. The new values for the elements of the apsidal motion were derived. We find periods of apsidal motion of about 255, 7000, 79.4 and 4400 years for V871 Aql, V345 Lac, V401 Lac and CR Set, respectively.
dc.identifier.doi10.1051/0004-6361:20035927
dc.identifier.wos000222606200023


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  • Publikační činnost VŠB-TUO / Publications of VŠB-TUO [2684]
    Kolekce obsahuje bibliografické záznamy publikační činnosti (článků) akademických pracovníků VŠB-TUO v časopisech (a v Lecture Notes in Computer Science) registrovaných ve Web of Science od roku 1990 po současnost.

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