Accretion Disk Models with Self-Consistent Advective Cooling and Heating

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dc.creatorArtemova, I. V.
dc.creatorBisnovatyi-Kogan, G. S.
dc.creatorBjornsson, G.
dc.creatorNovikov, I.
dc.date1996-01-03
dc.date.accessioned2026-07-07T02:20:42Z
dc.date.available2026-07-07T02:20:42Z
dc.descriptionWe present solutions to the accretion disk structure equations in which advective cooling is accounted for in a self-consistent way. It is shown that for high rates of accretion, above a critical value, when without advection there are no solutions extending continuously from large to small radii, there exist global solutions with self-consistent advective cooling. These solutions are quite different fromthose solutions obtained earlier by other authors, where advective cooling was not treated self-consistently.
dc.description9 pages, 4 figures, tarred and gzipped. Uses aasms4.sty
dc.identifierhttps://arxiv.org/abs/astro-ph/9601008
dc.identifierhttp://arxiv.org/abs/astro-ph/9601008
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10297
dc.subjectAstrophysics
dc.titleAccretion Disk Models with Self-Consistent Advective Cooling and Heating
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