Suzaku View of Magnetic Cataclysmic Variables

dc.contributor.author	Yuasa, T.
dc.date.accessioned	2023-01-18T14:25:25Z
dc.date.available	2023-01-18T14:25:25Z
dc.date.issued	2015
dc.identifier.citation	Acta Polytechnica. 2015, vol. 2, no. 1, p. 99-102.
dc.identifier.issn	1210-2709 (print)
dc.identifier.issn	1805-2363 (online)
dc.identifier.uri	http://hdl.handle.net/10467/105762
dc.description.abstract	Results of magnetic cataclysmic variable studies performed with the Suzaku satellite are reviewed in this article. Particular emphasis is placed on the recent update of X-ray spectral model of intermediate polars, possible kinematically redshifted fluorescent Fe K emission lines, and the magnetic CV contribution to the Galactic ridge X-ray emission.	en
dc.format.mimetype	application/pdf
dc.language.iso	eng
dc.publisher	České vysoké učení technické v Praze	cs
dc.publisher	Czech Technical University in Prague	en
dc.relation.ispartofseries	Acta Polytechnica
dc.relation.uri	https://ojs.cvut.cz/ojs/index.php/APP/article/view/2847
dc.rights	Creative Commons Attribution 4.0 International License	en
dc.rights.uri	http://creativecommons.org/licenses/by/4.0/
dc.title	Suzaku View of Magnetic Cataclysmic Variables
dc.type	article	en
dc.date.updated	2023-01-18T14:25:25Z
dc.identifier.doi	10.14311/APP.2015.02.0099
dc.rights.access	openAccess
dc.type.status	Peer-reviewed
dc.type.version	publishedVersion

Kromě případů, kde je uvedeno jinak, licence tohoto záznamu je Creative Commons Attribution 4.0 International License