1/2 Law for Non-Radiative Accretion Flow

Simple item page
dc.creatorGruzinov, Andrei
dc.date2001-04-06
dc.date.accessioned2026-07-07T01:58:09Z
dc.date.available2026-07-07T01:58:09Z
dc.descriptionAt low densities, when radiation of an accreting gas is dynamically unimportant, quasi-spherical non-radiative accretion flow is formed around a compact object. We show that the density of the flow is n\propto r^{-1/2}. The gas compression is much weaker than the standard Bondi's, n\propto r^{-3/2}, because most of the gas does not reach the compact object. It can either circulate indefinitely long or it can be launched to infinity.
dc.description4 pages, submitted to ApJL
dc.identifierhttps://arxiv.org/abs/astro-ph/0104113
dc.identifierhttp://arxiv.org/abs/astro-ph/0104113
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2661
dc.subjectAstrophysics
dc.title1/2 Law for Non-Radiative Accretion Flow
dc.typetext

Files

Collections

arXiv