Light-curve synthesis for close binaries overfilling their inner Roche lobes

dc.contributor.author	Mikhailishin V.
dc.date.accessioned	2018-09-17T21:10:34Z
dc.date.available	2018-09-17T21:10:34Z
dc.date.issued	2002
dc.identifier.issn	1063-7729
dc.identifier.uri	https://dspace.kpfu.ru/xmlui/handle/net/134627
dc.description.abstract	We present a procedure for calculating theoretical monochromatic light curves of close binary systems overfilling their inner Roche lobes. The close binaries are considered in a Roche model with a cold spot on one of the components. The system radiation is calculated in both a blackbody approximation and using model stellar atmospheres, taking into account tidal deformations of the components, limb darkening, gravitational darkening, and the effect of mutual heating of the components. © 2002 MAIK "Nauka/Interperiodica".
dc.relation.ispartofseries	Astronomy Reports
dc.title	Light-curve synthesis for close binaries overfilling their inner Roche lobes
dc.type	Article
dc.relation.ispartofseries-issue	9
dc.relation.ispartofseries-volume	46
dc.collection	Публикации сотрудников КФУ
dc.relation.startpage	740
dc.source.id	SCOPUS10637729-2002-46-9-SID0036756012

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