The Be X-ray Binary Outburst Zoo II

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dc.contributor.authorKühnel, M.
dc.contributor.authorKretschmar, P.
dc.contributor.authorNespoli, E.
dc.contributor.authorOkazaki, A.
dc.contributor.authorSchoenherr, G.
dc.contributor.authorWilson-Hodge, C.
dc.contributor.authorFalkner, S.
dc.contributor.authorBrand, T.
dc.contributor.authorAnders, F.
dc.contributor.authorSchwarm, F.
dc.contributor.authorKreykenbohm, I.
dc.contributor.authorMueller, S.
dc.contributor.authorPottschmidt, Katja
dc.contributor.authorFuerst, F.
dc.contributor.authorGrinberg, V.
dc.contributor.authorWilms, J.
dc.date.accessioned2023-09-06T14:03:44Z
dc.date.available2023-09-06T14:03:44Z
dc.date.issued2015-03-16
dc.description10th INTEGRAL Workshop: "A Synergistic View of the High Energy Sky" - Integral2014, 15-19 September 2014, Annapolis, MD, USAen_US
dc.description.abstractWe have continued our recently started systematic study of Be X-ray binary (BeXRB) outbursts. Specifically, we are developing a catalogue of outbursts including their basic properties based on nearly all available X-ray all-sky-monitors. These properties are derived by fitting asymmetric Gaussians to the outburst lightcurves. This model describes most of the outbursts covered by our preliminary catalogue well; only 13% of all datasets show more complex outburst shapes. Analyzing the basic properties, we reveal a strong correlation between the outburst length and the reached peak flux. As an example, we discuss possible models describing the observed correlation in EXO 2030+375en_US
dc.description.sponsorshipM. Kühnel acknowledges funding by the Bundesministerium für Wirtschaft und Technologie under Deutsches Zentrum für Luft- und Raumfahrt grant 50OR1113. The figures shown in this paper were created using the SLXfig module, which was developed by John E. Davis. We thank the organizers of the 10th Integral Workshop “A Synergistic View of the High Energy Sky” for the the useful discussions triggered by this interesting and well organized workshopen_US
dc.description.urihttps://pos.sissa.it/228/078/en_US
dc.format.extent10 pagesen_US
dc.genreconference papers and proceedingsen_US
dc.identifierdoi:10.13016/m2vbai-xqhw
dc.identifier.citationKühnel, Matthias, Peter Kretschmar, Elisa Nespoli, Atsuo Okazaki, Gabriele Schoenherr, Colleen Wilson-Hodge, Sebastian Falkner, et al. “The Be X-Ray Binary Outburst Zoo II.” In Proceedings of 10th INTEGRAL Workshop: A Synergistic View of the High-Energy Sky — PoS(Integral2014), 228:078. SISSA Medialab, 2015. https://doi.org/10.22323/1.228.0078.en_US
dc.identifier.urihttps://doi.org/10.22323/1.228.0078
dc.identifier.urihttp://hdl.handle.net/11603/29566
dc.language.isoen_USen_US
dc.publisherProceedings of Scienceen_US
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 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_US
dc.rightsPublic Domain Mark 1.0*
dc.rights.urihttp://creativecommons.org/publicdomain/mark/1.0/*
dc.titleThe Be X-ray Binary Outburst Zoo IIen_US
dc.typeTexten_US
dcterms.creatorhttps://orcid.org/0000-0002-4656-6881en_US

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