Broadband X-ray spectrum of the intermediate polar V2400 Oph

dc.contributor.author	Revnivtsev M.
dc.contributor.author	Lutovinov A.
dc.contributor.author	Suleimanov B.
dc.contributor.author	Molkov S.
dc.contributor.author	Sunyaev R.
dc.date.accessioned	2018-09-17T21:11:33Z
dc.date.available	2018-09-17T21:11:33Z
dc.date.issued	2004
dc.identifier.issn	1063-7737
dc.identifier.uri	https://dspace.kpfu.ru/xmlui/handle/net/134649
dc.description.abstract	We present the results of our analysis of the observations of the intermediate polar V2400 Oph by the INTEGRAL and RXTE observatories. We reconstructed the spectrum of the source over a wide (3-100 keV) energy range. The spectrum obtained can be fitted by a computed theoretical model of the post-shock emitting region with Tmax ∼ 22 keV. As a result, we estimated the mass (0.59M⊙) and radius (8.8 × 10 8 cm) of the white dwarf in the system V2400 Oph. © 2004 MAIK "Nauka/Interperiodica".
dc.relation.ispartofseries	Astronomy Letters
dc.subject	White dwarfs
dc.subject	X-ray sources
dc.title	Broadband X-ray spectrum of the intermediate polar V2400 Oph
dc.type	Article
dc.relation.ispartofseries-issue	11
dc.relation.ispartofseries-volume	30
dc.collection	Публикации сотрудников КФУ
dc.relation.startpage	772
dc.source.id	SCOPUS10637737-2004-30-11-SID10844230849

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