GRS 1758-258: Into the thermal dominant state with Swift XRT

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dc.contributor.authorHirsch, M.
dc.contributor.authorPottschmidt, Katja
dc.contributor.authorKrauss, F.
dc.contributor.authorEikmann, W.
dc.contributor.authorKreykenbohm, I.
dc.contributor.authorWilms, J.
dc.contributor.authorKuehnel, M.
dc.contributor.authorRodrigues, B. H. G.
dc.contributor.authorSoria, R.
dc.contributor.authorGrinberg, V.
dc.contributor.authorSmith, D. M.
dc.contributor.authorBel, M. Cadolle
dc.contributor.authorTomsick, J. A.
dc.contributor.authorBodaghee, A.
dc.contributor.authorKuulkers, E.
dc.contributor.authorKalemci, E.
dc.contributor.authorMiller, J. M.
dc.date.accessioned2023-08-31T16:54:07Z
dc.date.available2023-08-31T16:54:07Z
dc.date.issued2016-12-21
dc.description.urihttps://astronomerstelegram.org/?read=9890en_US
dc.format.extent2 pagesen_US
dc.genrearticlesen_US
dc.identifierdoi:10.13016/m2fpck-dgzm
dc.identifier.citationHirsch, M. et al. “GRS 1758-258: Into the thermal dominant state with Swift XRT”. ATel.9890,(21 Dec 2016). https://astronomerstelegram.org/?read=9890en_US
dc.identifier.urihttp://hdl.handle.net/11603/29490
dc.language.isoen_USen_US
dc.publisherThe Astronomer's Telegramen_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 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_US
dc.subjectX-rayen_US
dc.subjectBlack Holeen_US
dc.titleGRS 1758-258: Into the thermal dominant state with Swift XRTen_US
dc.typeTexten_US
dcterms.creatorhttps://orcid.org/0000-0002-4656-6881en_US

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