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dc.contributor.authorPatterson, Joseph
dc.contributor.authorMiguel Agustino, Enrique de 
dc.contributor.authorKemp, Jonathan
dc.contributor.authorDvorak, Shawn
dc.date.accessioned2020-10-15T07:28:46Z
dc.date.available2020-10-15T07:28:46Z
dc.date.issued2020-07
dc.identifier.citationPatterson, J., de Miguel Agustino, E., Kemp, J. ... Dvorak, S. (2020). The Spin-period History of Intermediate Polars. The Astrophysical Journal, 897(1), 70. DOI: https://doi.org/10.3847/1538-4357/ab863des_ES
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/10272/18908
dc.description.abstractWe report the detailed history of spin-period changes in five intermediate polars (DQ Herculis, AO Piscium, FO Aquarii, V1223 Sagittarii, and BG Canis Minoris) during the 30–60 yr since their original discovery. Most are slowly spinning up, although there are sometimes years-long episodes of spin-down. This is supportive of the idea that the underlying magnetic white dwarfs are near spin equilibrium. In addition to the 40 stars sharing many properties and defined by their strong, pulsed X-ray emission, there are a few rotating much faster (P<80 s), whose membership in the class is still in doubt—and who are overdue for closer study.es_ES
dc.language.isoenges_ES
dc.publisherAmerican Astronomical Societyes_ES
dc.relation.isversionofPublisher’s versión
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 España*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/*
dc.subject.otherCataclysmic variable starses_ES
dc.subject.otherClassical novaees_ES
dc.subject.otherClose binary starses_ES
dc.subject.otherDQ Herculis starses_ES
dc.subject.otherInteracting binary starses_ES
dc.subject.otherNovaees_ES
dc.subject.otherStellar accretiones_ES
dc.subject.otherStellar accretion diskses_ES
dc.titleThe Spin-period History of Intermediate Polarses_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.identifier.doi10.3847/1538-4357/ab863d
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses_ES


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