On the absence of winds in advection-dominated accretion flows

Monthly Notices of the Royal Astronomical Society

Volumn 314, Issue 4, 2000, Pages 775-781

  Abramowicz, Marek A ^a,b,c   Lasota, Jean Pierre ^a,e   Igumenshchev, Igor V ^b,d  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b UNIVERSITY OF GOTHENBURG   (Sweden)

^c SISSA   (Italy)

^d INSTITUTE OF ASTRONOMY   (Russian Federation)

^e CNRS   (France)

Author keywords

Accretion, accretion discs; Black hole physics; Hydrodynamics

Indexed keywords

ADVECTION; BLACK HOLES; EQUATIONS OF STATE; GRAVITATION; NUMERICAL MODELS; STARS; WIND;

ACCRETION FLOW; ACCRETION: ACCRETION DISKS; ADVECTION-DOMINATED ACCRETION FLOWS; BERNOULLI FUNCTION; BLACK HOLE PHYSICS; LOW RATES; LOW VISCOSITY; PROPERTY; RADIATIVE EFFICIENCY; STRONG WINDS;

VISCOSITY;

EID: 0000258623     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2000.03406.x     Document Type: Article

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