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
dc.format.extent2 pagesen
dc.genrearticlesen
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
dc.identifier.urihttp://hdl.handle.net/11603/29490
dc.language.isoenen
dc.publisherThe Astronomer's Telegramen
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.subjectX-rayen
dc.subjectBlack Holeen
dc.titleGRS 1758-258: Into the thermal dominant state with Swift XRTen
dc.typeTexten
dcterms.creatorhttps://orcid.org/0000-0002-4656-6881en

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