Be-Phenomenon in Neutron Star X-ray Binaries

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dc.contributor.authorKühnel, M.
dc.contributor.authorKretschmar, P.
dc.contributor.authorFürst, F.
dc.contributor.authorPottschmidt, Katja
dc.contributor.authorHemphill, P.
dc.contributor.authorRothschild, R. E.
dc.contributor.authorOkazaki, A. T.
dc.contributor.authorSagredo, M.
dc.contributor.authorWilms, J.
dc.date.accessioned2023-08-31T16:50:56Z
dc.date.available2023-08-31T16:50:56Z
dc.date.issued2017
dc.description.abstractIn this work we provide a brief insight into two aspects of Be/X-ray binaries, which are probably involved in production of X-ray outbursts: the evolution of the Be star disk, in particular of its size, and the binary geometry which drives gravitational interaction. Simultaneous X-ray and optical data will aid our investigation of the evolution of Be stars in binaries and the X-ray outburst mechanism.en
dc.description.sponsorshipMK acknowledges funding by the European Space Agency under contract 4000115860/15/NL/IB.en
dc.description.urihttp://aspbooks.org/custom/publications/paper/508-0385.htmlen
dc.genrejournal articlesen
dc.identifierdoi:10.13016/m2ypk9-50xj
dc.identifier.citationKühnel, M., et al. "Be-Phenomenon in Neutron Star X-ray Binaries." The B[e] Phenomenom: Forty Years of Studies 508 (2017): 385. http://aspbooks.org/custom/publications/paper/508-0385.html.en
dc.identifier.urihttp://hdl.handle.net/11603/29487
dc.language.isoenen
dc.publisherAstronomical Society of the Pacificen
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Center for Space Sciences and Technology
dc.relation.ispartofUMBC Physics Department
dc.relation.ispartofUMBC Faculty Collection
dc.rightsThis item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author.en
dc.subjectBe-Phenomenonen
dc.subjectBe X-ray Binariesen
dc.subjectX-ray / Hα Connectionen
dc.subjectTidal Interactionsen
dc.titleBe-Phenomenon in Neutron Star X-ray Binariesen
dc.typeTexten
dcterms.creatorhttps://orcid.org/0000-0002-4656-6881en

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