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Analytic Model for Advection‐dominated Accretion Flows in a Global Magnetic Field
Author(s) -
Osamu Kaburaki
Publication year - 2000
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/308442
Subject(s) - advection , accretion (finance) , physics , magnetic field , angular momentum , mechanics , flow (mathematics) , dissipation , classical mechanics , astrophysics , thermodynamics , quantum mechanics
A model for advection-dominated accretion flows (ADAFs) in a global magneticfield is proposed. In contrast to the well known ADAF models in which theviscosity of a fluid determines both angular momentum transfer and energydissipation in the flow, the magnetic field and the electric resistivity,respectively, control them in this model. A manageable set of analyticsolutions for the flow and the magnetic field is obtained to verticallynon-integrated basic equations. This set describes mathematically a fullyadvective accretion flow and, in physically plausible situations for most AGNs,it is also confirmed that the radiation cooling estimated on this solution isreally negligible compared with the internal energy of the flow.Comment: 27pages, 1 figure, to appear in ApJ vol 529, Feb.1, 200

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