On the morphology of accretion flows with small, non-zero specific angular momentum

Monthly Notices of the Royal Astronomical Society

Volumn 285, Issue 2, 1997, Pages 439-448

  Chen, Xingming ^a,b   Taam, Ronald E ^a   Abramowicz, Marek A ^b   Igumenshchev, Igor V ^b,c  

^a NORTHWESTERN UNIVERSITY   (United States)

^b UNIVERSITY OF GOTHENBURG   (Sweden)

^c INSTITUTE OF ASTRONOMY   (Russian Federation)

Author keywords

Accretion, accretion discs; Hydrodynamics; Methods: numerical

Indexed keywords

NUMERICAL METHODS; SHOCK WAVES;

ACCRETION FLOW; ACCRETION: ACCRETION DISKS; AXISYMMETRIC; EQUATORIAL PLANES; INCOMING FLOWS; INITIAL STATE; METHOD: NUMERICAL; POLAR ANGLES; SHOCK STRUCTURE; VISCOUS LIMITS;

ANGULAR MOMENTUM;

EID: 0009124706     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/285.2.439     Document Type: Article

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