Supersoft X-ray sources: Basic parameters

dc.contributor.author	Suleǐmanov V.
dc.contributor.author	Ibragimov A.
dc.date.accessioned	2018-09-17T21:10:38Z
dc.date.available	2018-09-17T21:10:38Z
dc.date.issued	2003
dc.identifier.issn	1063-7729
dc.identifier.uri	https://dspace.kpfu.ru/xmlui/handle/net/134629
dc.description.abstract	The parameters of ten supersoft X-ray sources observed by ROSAT obtained using blanketing approximations and LTE model atmospheres are analyzed. The consistency of the resulting parameters with a model with stable/recurrent burning on the surface of the white dwarf is studied. The luminosity and sizes of seven of the sources are in good agreement with this model. The masses of the white dwarfs in these sources are estimated. A formula that can be used to estimate the masses of white dwarfs in classical super-soft sources based on their effective temperatures is presented. © 2003 MAIK "Nauka/Interperiodica".
dc.relation.ispartofseries	Astronomy Reports
dc.title	Supersoft X-ray sources: Basic parameters
dc.type	Article
dc.relation.ispartofseries-issue	3
dc.relation.ispartofseries-volume	47
dc.collection	Публикации сотрудников КФУ
dc.relation.startpage	197
dc.source.id	SCOPUS10637729-2003-47-3-SID0345381896

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