The Inner Boundary Condition for a Thin Disk Accreting Into a Black Hole

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dc.creatorPaczyński, B.
dc.date2000-04-10
dc.date.accessioned2026-07-07T01:53:05Z
dc.date.available2026-07-07T01:53:05Z
dc.descriptionContrary to some recent claims the `no torque inner boundary condition' as applied at the marginally stable orbit is correct for geometrically thin disks accreting into black holes.
dc.description3 pages, latex, submitted on April 10, 2000 to The Astrophysical Journal Letters
dc.identifierhttps://arxiv.org/abs/astro-ph/0004129
dc.identifierhttp://arxiv.org/abs/astro-ph/0004129
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/843
dc.subjectAstrophysics
dc.titleThe Inner Boundary Condition for a Thin Disk Accreting Into a Black Hole
dc.typetext

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