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INTEGRAL View on cataclysmic variables and symbiotic binaries

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dc.contributor.authorLutovinov, Alexander
dc.contributor.authorSuleimanov, Valery
dc.contributor.authorSazonov, Sergey
dc.contributor.authorMartino, Domitilla de
dc.contributor.authorDucci, Lorenzo
dc.contributor.authorDoroshenko, Victor
dc.contributor.authorFalanga, Maurizio
dc.date.accessioned2025-01-30T15:57:42Z
dc.date.available2025-01-30T15:57:42Z
dc.date.issued2020
dc.description.abstractAccreting white dwarfs (WDs) constitute a significant fraction of the hard X-ray sources detected by the INTEGRAL observatory. Most of them are magnetic Cataclysmic Variables (CVs) of the intermediate polar (IP) and polar types, but the contribution of the Nova-likes systems and the systems with optically thin boundary layers, Dwarf Novae (DNs) and Symbiotic Binaries (or Symbiotic Stars, SySs) in quiescence is also not negligible. Here we present a short review of the results obtained from the observations of cataclysmic variables and symbiotic binaries by INTEGRAL. The highlight results include the significant increase of the known IP population, determination of the WD mass for a significant fraction of IPs, the establishment of the luminosity function of magnetic CVs, and uncovering origin of the Galactic ridge X-ray emission which appears to largely be associated with hard emission from magnetic CVs
dc.description.filiationFil: Lutovinov, Alexander. Space Research Institute; Rusia. Moscow Institute of Physics and Technology; Rusia
dc.description.filiationFil: Suleimanov, Valery. Eberhard Karls Universität Tübingen; Alemania. Space Research Institute; Rusia. Kazan Federal University; Rusia
dc.description.filiationFil: Luna, Gerardo Juan Manuel. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina. Universidad Nacional de Hurlingham. Instituto de Tecnología e Ingeniería; Argentina
dc.description.filiationFil: Sazonov, Sergey. Space Research Institute; Rusia. Moscow Institute of Physics and Technology; Rusia
dc.description.filiationFil: Martino, Domitilla de. Istituto Nazionale di Astrofisica; Italia
dc.description.filiationFil: Ducci, Lorenzo. Eberhard Karls Universität Tübingen; Alemania. Universidad de Genova; España
dc.description.filiationFil: Doroshenko, Victor. Space Research Institute; Rusia. Eberhard Karls Universität Tübingen; Alemania
dc.description.filiationFil: Falanga, Maurizio. International Space Science Institute; Suiza
dc.format.mimetypeapplication/pdf
dc.identifier.citationLutovinov, Alexander; Suleimanov, Valery; Luna, Gerardo Juan Manuel; Sazonov, Sergey; Martino, Domitilla de; et al. (2020) INTEGRAL View on cataclysmic variables and symbiotic binaries, New Astronomy Reviews, 91, (101547), pp. 1-14
dc.identifier.doihttp://dx.doi.org/10.1016/j.newar.2020.101547
dc.identifier.issn1387-6473
dc.identifier.urihttps://www.sciencedirect.com/science/article/pii/S1387647320300245
dc.identifier.urihttps://repositorio.unahur.edu.ar/handle/123456789/523
dc.journal.number101547
dc.journal.pagination1-14
dc.journal.titleNew Astronomy Reviews
dc.journal.volume91
dc.language.isoeng
dc.publisherElsevier
dc.rights.licenseinfo:eu-repo/semantics/restrictedAccess
dc.subject.ocde1Ciencias Exactas y Naturales
dc.subject.ocde2Ciencias Físicas
dc.subject.unahurCiencias Básicas y Aplicadas
dc.titleINTEGRAL View on cataclysmic variables and symbiotic binaries
dc.typeinfo:eu-repo/semantics/article
dc.type.oaireinfo:eu-repo/semantics/article
dc.type.snrdinfo:ar-repo/semantics/artículo
dc.type.versioninfo:eu-repo/semantics/publishedVersion
dspace.entity.typePublication
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