Atmospheres and spectra of X-ray illuminated stars: A gray model

dc.contributor.author	Sakhibullin N.
dc.contributor.author	Shimanskii V.
dc.date.accessioned	2018-09-17T21:09:58Z
dc.date.available	2018-09-17T21:09:58Z
dc.date.issued	1996
dc.identifier.issn	1063-7729
dc.identifier.uri	https://dspace.kpfu.ru/xmlui/handle/net/134611
dc.description.abstract	A gray model is used to explore the effect of heating of stellar atmospheres by an external X-ray flux. This flux is shown to produce additional heating functions in the surface and inner layers. The opacity sources in the X-ray region are determined. A technique for calculating the reflection effect in the gray approximation is presented. The illuminated and normal atmospheres and their spectra are shown to differ considerably.
dc.relation.ispartofseries	Astronomy Reports
dc.title	Atmospheres and spectra of X-ray illuminated stars: A gray model
dc.type	Article
dc.relation.ispartofseries-issue	1
dc.relation.ispartofseries-volume	40
dc.collection	Публикации сотрудников КФУ
dc.relation.startpage	62
dc.source.id	SCOPUS10637729-1996-40-1-SID0030522085

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Коллекция содержит публикации сотрудников Казанского федерального (до 2010 года Казанского государственного) университета, проиндексированные в БД Scopus, начиная с 1970г.