Influence of rotation velocity gradient on line profiles of accretion discs of CVs

dc.contributor.author	Korčáková D.
dc.contributor.author	Nagel T.
dc.contributor.author	Werner K.
dc.contributor.author	Suleimanov V.
dc.contributor.author	Votruba V.
dc.date.accessioned	2018-09-18T20:25:40Z
dc.date.available	2018-09-18T20:25:40Z
dc.date.issued	2011
dc.identifier.issn	1743-9213
dc.identifier.uri	https://dspace.kpfu.ru/xmlui/handle/net/139765
dc.description.abstract	We show the influence of the Keplerian velocity shear on the line profiles of cataclysmic variable discs. The complete disc structure is taken into account. The radial disc structure follows the alpha disc approximation. Based on this assumption, the vertical structure is computed using the detailed non-LTE code AcDc. The obtained opacities and source functions are interpolated in the 2D grid, where the radiative transfer is calculated with the inclusion of the velocity field gradient. © International Astronomical Union 2012.
dc.relation.ispartofseries	Proceedings of the International Astronomical Union
dc.subject	accretion disks
dc.subject	cataclysmic variables
dc.subject	line: formation
dc.subject	methods: numerical
dc.title	Influence of rotation velocity gradient on line profiles of accretion discs of CVs
dc.type	Conference Paper
dc.relation.ispartofseries-issue	S282
dc.relation.ispartofseries-volume	7
dc.collection	Публикации сотрудников КФУ
dc.relation.startpage	255
dc.source.id	SCOPUS17439213-2011-7-282-SID84887363564

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Публикации сотрудников КФУ Scopus [24551]
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