Accretion Disk Models

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dc.creatorBeloborodov, Andrei M.
dc.date1999-01-10
dc.date.accessioned2026-07-07T02:29:55Z
dc.date.available2026-07-07T02:29:55Z
dc.descriptionModels of black hole accretion disks are reviewed, with an emphasis on the theory of hard X-ray production. The following models are considered: i) standard, ii) super-critical, iii) two-temperature, and iv) disk+corona. New developments have recently been made in hydrodynamical models of accretion and in phenomenological radiative models fitting the observed X-ray spectra. Attempts to unify the two approaches are only partly successful.
dc.description20 pages. Invited review at the workshop ``High Energy Processes in Accreting Black Holes'', eds. J. Poutanen & R. Svensson, ASP Conf. Series, in press
dc.identifierhttps://arxiv.org/abs/astro-ph/9901108
dc.identifierhttp://arxiv.org/abs/astro-ph/9901108
dc.identifierASP Conf.Ser. 161 (1999) 295
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13659
dc.subjectAstrophysics
dc.titleAccretion Disk Models
dc.typetext

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