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dc.contributor.authorZhou, X.
dc.contributor.authorSoria, Roberto
dc.date.accessioned2017-01-30T12:22:44Z
dc.date.available2017-01-30T12:22:44Z
dc.date.created2016-02-17T19:30:19Z
dc.date.issued2012
dc.identifier.citationZhou, X. and Soria, R. 2012. Black hole masses from X-rays. Proceedings of the International Astronomical Union. 8 (S290): pp. 371-372.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/21034
dc.identifier.doi10.1017/S1743921312020455
dc.description.abstract

We discuss two methods to estimate black hole (BH) masses using X-ray data only: from the X-ray variability amplitude and from the photon index G. The first method is based on the anti-correlation between BH mass and X-ray variability amplitude. Using a sample of AGN with BH masses from reverberation mapping, we show that this method shows small intrinsic scatter. The second method is based on the correlation between G and both the Eddington ratio L bol/L Edd and the bolometric correction L bol/L 2-10keV. © International Astronomical Union 2013.

dc.titleBlack hole masses from X-rays
dc.typeConference Paper
dcterms.source.volume8
dcterms.source.startPage371
dcterms.source.endPage372
dcterms.source.titleProceedings of the International Astronomical Union
dcterms.source.seriesProceedings of the International Astronomical Union
dcterms.source.isbn9781107033795
curtin.departmentDepartment of Physics and Astronomy
curtin.accessStatusOpen access via publisher


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