Towards steady-state solutions for supersonic wind accretion on to gravitating objects

Monthly Notices of the Royal Astronomical Society

Volumn 313, Issue 1, 2000, Pages 198-208

  Pogorelov, N V ^a,b   Ohsugi, Y ^b   Matsuda, T ^b  

^a INSTITUTE FOR PROBLEMS IN MECHANICS   (Russian Federation)

^b KOBE UNIVERSITY   (Japan)

Author keywords

Accretion, accretion discs; Black hole physics; Hydrodynamics; Instabilities; Methods: numerical; Shock waves

Indexed keywords

BLACK HOLES; NUMERICAL METHODS; RELATIVITY; SHOCK WAVES; STARS;

ACCRETION: ACCRETION DISKS; AXISYMMETRIC; BLACK HOLE PHYSICS; CORRECTION PROCEDURE; HIGH RESOLUTION; METHOD: NUMERICAL; NUMERICAL SCHEME; SHOCK-WAVES; STEADY STATE SOLUTION; SUPERSONIC WIND ACCRETION;

HYDRODYNAMICS;

EID: 0001663810     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2000.03199.x     Document Type: Article

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