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dc.contributor.authorAndronov, Ivan L.-
dc.contributor.authorAndrych, K. D.-
dc.date.accessioned2015-02-24T08:45:19Z-
dc.date.available2015-02-24T08:45:19Z-
dc.date.issued2014-
dc.identifier.citationOdessa Astronomical Publicationsuk
dc.identifier.urihttp://dspace.onu.edu.ua:8080/handle/123456789/5906-
dc.descriptionOdessa Astronomical publications / Одесская астроном. обсерватория . – Одесса : Астропринт, 2014 . – Vol.27, I. 1.uk
dc.description.abstractThe dependencies of the phase of eclipse of the white dwarf’s centre and the durations of the ascending and descending branches of the light curve on the binary system’s parameters were computed using the sphericallysymmetric approximation and the more accurate model of the elliptical projection onto the celestial sphere of the companion (red dwarf) that fills its Roche lobe. The parameters of eclipses in the classical eclipsing polar OTJ 071126+440405 = CSS 081231:071126+440405 were estimated.uk
dc.language.isoenuk
dc.publisherAstroprintuk
dc.relation.ispartofseries;V. 27, I. 1, P. 38-40.-
dc.subjectStarsuk
dc.subjectvariable – starsuk
dc.subjectbinary – starsuk
dc.subjectcataclysmicuk
dc.titleDetermination of size of the emitting region in eclipsing cataclysmic variable starsuk
dc.typeArticleuk
Appears in Collections:Odessa Astronomical Publications

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