Collisionless Halos Around Black Holes

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dc.creatorGruzinov, Andrei
dc.date1999-08-04
dc.date.accessioned2026-07-07T02:32:43Z
dc.date.available2026-07-07T02:32:43Z
dc.descriptionWhen a black hole accretes slowly, the radiative cooling of the infalling gas is weak and the accretion disk does not form. A hot collisionless quasi-spherical halo is formed instead. The properties of such halos are discussed. The rate of accretion, the radiative efficiency, and the temperature and density near the hole are evaluated.
dc.description7 pages, Proceedings IAU Symposium 195
dc.identifierhttps://arxiv.org/abs/astro-ph/9908027
dc.identifierhttp://arxiv.org/abs/astro-ph/9908027
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14562
dc.subjectAstrophysics
dc.titleCollisionless Halos Around Black Holes
dc.typetext

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