Statistics of white dwarf properties in intermediate polars

dc.contributor.author	Suleimanov V.F.
dc.contributor.author	Doroshenko V.A.
dc.contributor.author	Werner K.
dc.date.accessioned	2021-02-25T20:46:18Z
dc.date.available	2021-02-25T20:46:18Z
dc.date.issued	2020
dc.identifier.issn	1743-9213
dc.identifier.uri	https://dspace.kpfu.ru/xmlui/handle/net/162383
dc.description.abstract	© The Author(s), 2020. Many intermediate polars are hard X-ray sources. The theory of their hard X-ray radiation is well developed and allows us to determine white dwarf masse in this kind of cataclysmic variables. Here we present the results of determination of the masses of 35 white dwarfs in the intermediate polars observed by observatories NuSTAR (10 sources) and Swift/BAT (25 sources). The corresponding mass accrerion rates and the luminosity function were also derived due to accurate distances to the sources well known now after Gaia DR2.
dc.relation.ispartofseries	Proceedings of the International Astronomical Union
dc.subject	Cataclysmic variables
dc.subject	Mass function
dc.subject	Novae
dc.subject	Stars: Luminosity function
dc.subject	X-rays: Binaries
dc.title	Statistics of white dwarf properties in intermediate polars
dc.type	Article
dc.collection	Публикации сотрудников КФУ
dc.relation.startpage	202
dc.source.id	SCOPUS17439213-2020-SID85095437043

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