Accretion around supermassive black holes: the detection of the Balmer edge signature from quasars

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dc.creatorKishimoto, Makoto
dc.creatorAntonucci, Robert
dc.creatorBoisson, Catherine
dc.creatorBlaes, Omer
dc.date2004-02-26
dc.date.accessioned2026-07-07T10:47:48Z
dc.date.available2026-07-07T10:47:48Z
dc.descriptionThe ultraviolet/optical continuum of quasars is thought to be from an accretion flow around a supermassive black hole, and it dominates the radiative output of quasars. However, the nature of this emission, often called the Big Blue Bump, has not been well understood. Robust evidence for its thermal nature would be a continuum opacity edge feature intrinsic to this component, but this has not been clearly confirmed despite the predictions by many models. We are now developing and exploiting a new method to detect the Balmer edge of hydrogen opacity. The method overcomes for certain objects the major obstacle of the heavy contamination from emissions outside the nucleus by taking the polarized flux spectrum. If our interpretation of the polarized flux is correct, our data show that the Big Blue Bump emission has a Balmer edge in absorption, indicating that the emission is indeed thermal, and the emitter is optically thick.
dc.description4 pages, a talk contribution to the conference "Stellar-mass, Intermediate-mass, and Supermassive Black Holes", held in Kyoto, Japan, Octorber 28-31, 2003, to be published in Progress of Theoretical Physics Supplement
dc.identifierhttps://arxiv.org/abs/astro-ph/0402643
dc.identifierhttp://arxiv.org/abs/astro-ph/0402643
dc.identifierProg.Theor.Phys.Suppl.155:166-169,2004
dc.identifierdoi:10.1143/PTPS.155.166
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/183662
dc.subjectAstrophysics
dc.titleAccretion around supermassive black holes: the detection of the Balmer edge signature from quasars
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