Advection dominated flows around black holes in two dimensions

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dc.creatorLee, William H.
dc.date2000-11-07
dc.date.accessioned2026-07-07T01:56:27Z
dc.date.available2026-07-07T01:56:27Z
dc.descriptionWe show the results of two-dimensional, azimuthally symmetric simulations of advection dominated fluid flows around black holes. We use the SPH method, and the alpha-prescription for the viscosity, including all terms in the stress tensor. We have performed calculations with 0.001 < alpha < 0.2 and find strong circulation patterns in the flow, on spatial scales that depend on the magnitude of the viscosity.
dc.description2 pages, To be published in `Proceedings of the Third Microquasar Workshop: Granada Workshop on galactic relativistic jet sources', Eds: A. J. Castro-Tirado, J. Greiner and J. M. Paredes, Astrophysics and Space Science, in press
dc.identifierhttps://arxiv.org/abs/astro-ph/0011151
dc.identifierhttp://arxiv.org/abs/astro-ph/0011151
dc.identifierAstrophys.Space Sci. 276 (2001) 239-240
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2007
dc.subjectAstrophysics
dc.titleAdvection dominated flows around black holes in two dimensions
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