Physics of the Accretion Mound at the Magnetic Poles of Neutron Stars

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dc.contributor.authorRothschild, Richard E.
dc.contributor.authorStaubert, Rudiger
dc.contributor.authorWilms, Jorn
dc.contributor.authorSantangelo, Andrea
dc.contributor.authorKretschmar, Peter
dc.contributor.authorKreykenbohm, Ingo
dc.contributor.authorPottschmidt, Katja
dc.contributor.authorSchonherr, Gabrielle
dc.contributor.authorMcBride, Vanessa
dc.contributor.authorKendziorra, Eckhard
dc.contributor.authorShakura, Nikolai
dc.contributor.authorPostnov, Konstantin
dc.contributor.authorKlochkov, Dmitri
dc.contributor.authorNishimura, Osamu
dc.contributor.authorWilson-Hodge, Colleen
dc.contributor.authorWolff, Michael
dc.contributor.authorWood, Kent
dc.date.accessioned2023-10-04T21:11:20Z
dc.date.available2023-10-04T21:11:20Z
dc.description.abstractThe study of the physical processes in the region just above the magnetic poles of strongly magnetic accreting neutron stars is essential to the understanding of stellar and binary system evolution, as well as that of the origin and evolution of neutron star magnetic fields. Recent advances in modeling these processes have resulted in direct measurement of the magnetic fields and plasma parameters in physical units as opposed to empirical ones.en
dc.description.urihttps://www.nrao.edu/A2010/whitepapers/rac/rothschild_NS_cyclotron_line_continuum_SSE.pdfen
dc.format.extent7 pagesen
dc.genrewhite papersen
dc.identifierdoi:10.13016/m2so17-zqlm
dc.identifier.urihttp://hdl.handle.net/11603/29946
dc.language.isoenen
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Center for Space Sciences and Technology
dc.relation.ispartofUMBC Faculty Collection
dc.relation.ispartofUMBC Physics Department
dc.rightsPublic Domain Mark 1.0*
dc.rightsThis work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.en
dc.rights.urihttp://creativecommons.org/publicdomain/mark/1.0/*
dc.titlePhysics of the Accretion Mound at the Magnetic Poles of Neutron Starsen
dc.typeTexten
dcterms.creatorhttps://orcid.org/0000-0002-4656-6881en

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