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

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

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