Particle Heating in Advection-Dominated Accretion Flows

Simple item page
dc.creatorQuataert, Eliot
dc.date1998-09-25
dc.date.accessioned2026-07-07T02:28:04Z
dc.date.available2026-07-07T02:28:04Z
dc.descriptionI review particle heating by MHD turbulence in collisionless plasmas appropriate to advection-dominated accretion flows. These considerations suggest that the preferential turbulent heating of protons assumed by theoretical models is only achieved for relatively subthermal magnetic fields.
dc.description6 pages, uses paspconf.sty, to appear in Proc. of ``The Workshop on High Energy Processes in Accreting Black Holes,'' eds. J. Poutanen & R. Svensson
dc.identifierhttps://arxiv.org/abs/astro-ph/9809332
dc.identifierhttp://arxiv.org/abs/astro-ph/9809332
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12962
dc.subjectAstrophysics
dc.titleParticle Heating in Advection-Dominated Accretion Flows
dc.typetext

Files

Collections

arXiv