Radiatively inefficient accretion disks

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dc.creatorSpruit, H. C.
dc.date2000-03-10
dc.date2000-03-31
dc.date.accessioned2026-07-07T01:52:41Z
dc.date.available2026-07-07T01:52:41Z
dc.descriptionRadiatively inefficient (or advection dominated) disks are discussed at an introductory level. Ion supported and radiation supported flows are discussed, the different consequences of advection dominated flows onto black holes vs. solid surfaces (neutron stars, white dwarfs), hydrodynamics, the role of the ratio of specific heats, and the possible connection between ADAFs and outflows.
dc.descriptionTo appear in: The neutron star black hole connection (NATO ASI ELOUNDA 1999) ed. C. Kouveliotou et al. New version: typos and other corrections
dc.identifierhttps://arxiv.org/abs/astro-ph/0003143
dc.identifierhttp://arxiv.org/abs/astro-ph/0003143
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/702
dc.subjectAstrophysics
dc.titleRadiatively inefficient accretion disks
dc.typetext

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