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dc.contributor.authorNarayan, Ramesh
dc.contributor.authorRaymond, John
dc.date.accessioned2019-09-22T14:24:24Z
dc.date.issued1999
dc.identifier.citationNarayan, Ramesh, and John Raymond. 1999. “Thermal X-Ray Line Emission from Accreting Black Holes.” The Astrophysical Journal 515 (2): L69–72. https://doi.org/10.1086/311973.
dc.identifier.issn0004-637X
dc.identifier.issn1538-4357
dc.identifier.urihttp://nrs.harvard.edu/urn-3:HUL.InstRepos:41384921*
dc.description.abstractWe present model X-ray spectra of accreting black holes with hot advection-dominated accretion flows, paying attention to thermal emission lines from the hot plasma. We discuss the emission-line diagnostics that are potentially observable with the next generation of X-ray observatories, emphasizing the possibilities for determining the outer radius of the hot plasma, the presence of a wind, and the relative importance of photoionization. We present example spectra of V404 Cyg in quiescence, the Galactic center black hole Sagittarius A*, and the nucleus of M87.
dc.language.isoen_US
dc.publisherAmerican Astronomical Society
dash.licenseLAA
dc.titleThermal X-Ray Line Emission from Accreting Black Holes
dc.typeJournal Article
dc.description.versionAccepted Manuscript
dc.relation.journalThe Astrophysical Journal
dash.depositing.authorNarayan, Ramesh::dc7afe5d74d62c7b451015317ea2ccbe::600
dc.date.available2019-09-22T14:24:24Z
dash.workflow.comments1Science Serial ID 95668
dc.identifier.doi10.1086/311973
dash.source.volume515;2
dash.source.pageL69-L72


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