State-or-the-art Accretion and Wind Solutions Around Black Holes

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dc.creatorChakrabarti, Sandip K.
dc.date2000-12-29
dc.date.accessioned2026-07-07T01:57:12Z
dc.date.available2026-07-07T01:57:12Z
dc.descriptionWe report all possible basic solutions of an advective disk model and use them to explain major observations from black hole candidates.
dc.descriptionWorld Scientific Style (two pages with a figure)
dc.identifierhttps://arxiv.org/abs/astro-ph/0012530
dc.identifierhttp://arxiv.org/abs/astro-ph/0012530
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2293
dc.subjectAstrophysics
dc.titleState-or-the-art Accretion and Wind Solutions Around Black Holes
dc.typetext

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