X-ray variations in the inner accretion flow of dwarf novae

dc.contributor.author	BALMAN, Şölen
dc.contributor.author	Revnivtsev, M.
dc.date.accessioned	2021-03-04T10:38:50Z
dc.date.available	2021-03-04T10:38:50Z
dc.identifier.citation	BALMAN Ş., Revnivtsev M., "X-ray variations in the inner accretion flow of dwarf novae", ASTRONOMY & ASTROPHYSICS, cilt.546, 2012
dc.identifier.issn	1432-0746
dc.identifier.other	vv_1032021
dc.identifier.other	av_6e46fab9-bdb8-427c-a27b-a4d4e0617f69
dc.identifier.uri	http://hdl.handle.net/20.500.12627/76137
dc.identifier.uri	https://doi.org/10.1051/0004-6361/201219469
dc.description.abstract	Aims. We study the inner disk structure of dwarf novae (DNe; i.e., nonmagnetic cataclysmic variables).
dc.language.iso	eng
dc.subject	Astronomi ve Astrofizik
dc.subject	Temel Bilimler
dc.subject	Fizik
dc.subject	Temel Bilimler (SCI)
dc.subject	Uzay bilimi
dc.subject	ASTRONOMİ VE ASTROFİZİK
dc.title	X-ray variations in the inner accretion flow of dwarf novae
dc.type	Makale
dc.relation.journal	ASTRONOMY & ASTROPHYSICS
dc.contributor.department	Orta Doğu Teknik Üniversitesi , Fen Fakültesi , Astrofizik Ana Bilim Dalı
dc.identifier.volume	546
dc.contributor.firstauthorID	2212709

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