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dc.contributor.authorSutton, A.
dc.contributor.authorSwartz, D.
dc.contributor.authorRoberts, T.
dc.contributor.authorMiddleton, M.
dc.contributor.authorSoria, Roberto
dc.contributor.authorDone, C.
dc.date.accessioned2017-03-24T11:53:52Z
dc.date.available2017-03-24T11:53:52Z
dc.date.created2017-03-23T06:59:51Z
dc.date.issued2017
dc.identifier.citationSutton, A. and Swartz, D. and Roberts, T. and Middleton, M. and Soria, R. and Done, C. 2017. Crossing the Eddington Limit: Examining Disk Spectra at High Accretion Rates. Astrophysical Journal. 836: 48.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/51550
dc.identifier.doi10.3847/1538-4357/836/1/48
dc.description.abstract

The faintest ultraluminous X-ray sources (ULXs), those with 0.3-10 keV luminosities 1 < Lx/10 39 < 3 erg s-1, tend to have X-ray spectra that are disk-like but broader than expected for thin accretion disks. These "broadened disk (BD)" spectra are thought to indicate near- or mildly super-Eddington accretion onto stellar remnant black holes. Here we report that a sample of bright thermal-dominant black hole binaries, which have Eddington ratios constrained to moderate values, also show BD spectra in the 0.3-10 keV band at an order of magnitude lower luminosities. This broadening would be missed in studies that only look above ~ 2 keV. While this may suggest that BD ULXs could be powered by accretion onto massive stellar remnant black holes with close to maximal spin, we argue in favor of a scenario where they are at close to the Eddington luminosity, such that radiation pressure would be expected to result in geometrically slim, advective accretion disks. However, this implies that an additional physical mechanism is required to produce the observed broad spectra at low Eddington ratios. © 2017. The American Astronomical Society. All rights reserved

dc.publisherInstitute of Physics Publishing
dc.titleCrossing the Eddington Limit: Examining Disk Spectra at High Accretion Rates
dc.typeJournal Article
dcterms.source.volume836
dcterms.source.number1
dcterms.source.issn0004-637X
dcterms.source.titleAstrophysical Journal
curtin.note

Copyright © 2017 The American Astronomical Society. All rights reserved.

curtin.departmentCurtin Institute of Radio Astronomy (Physics)
curtin.accessStatusOpen access


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