Hard X-ray cataclysmic variables

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dc.contributor.authorde Martino, D.
dc.contributor.authorBernardini, F..
dc.contributor.authorMukai, K.
dc.contributor.authorFalanga, M.
dc.contributor.authorMasetti, N.
dc.date.accessioned2022-11-25T17:20:53Z
dc.date.available2022-11-25T17:20:53Z
dc.date.issued2020-09
dc.descriptionIndexación: Scopuses
dc.description.abstractAmong hard X-ray Galactic sources detected with the Swift and INTEGRAL surveys, those discovered as accreting white dwarf binaries have surprisingly boosted in number in the recent years. The majority are identified as magnetic Cataclysmic Variables of the Intermediate Polar type, suggesting this subclass as an important constituent of the Galactic population of X-ray sources. We here review and discuss the X-ray emission properties of newly discovered sources in the framework of an identification programme with the XMM-Newton satellite that increased the sample of this subclass by a factor of two. © 2019 COSPARes
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dc.identifier.doi10.1016/j.asr.2019.09.006
dc.identifier.issn0273-1177
dc.identifier.urihttps://repositorio.unab.cl/xmlui/handle/ria/24919
dc.language.isoenes
dc.publisherElsevier Ltdes
dc.rights.licenseAtribución 4.0 Internacional (CC BY 4.0)
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/deed.es
dc.subjectAccretiones
dc.subjectAccretion discses
dc.subjectStarses
dc.subjectcataclysmic variableses
dc.subjectX-Rayses
dc.subjectbinarieses
dc.titleHard X-ray cataclysmic variableses
dc.typeArtículoes
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Advances in Space Research Volume 66, Issue 5, Pages 1209 - 12251 September 2020
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