Extending the Shakura-Sunyaev approach to a strongly magnetized accretion disc model

Astronomy and Astrophysics

Volumn 407, Issue 2, 2003, Pages 403-421

  Pariev, V I ^a,b   Blackman, E G ^a   Boldyrev, S A ^c  

^a UNIVERSITY OF ROCHESTER   (United States)

^b LEBEDEV PHYSICAL INSTITUTE   (Russian Federation)

^c UNIVERSITY OF CHICAGO   (United States)

Author keywords

Accretion: accretion disks; Magnetohydrodynamics (MHD); Plasmas; Turbulence

Indexed keywords

CALCULATIONS; EMISSION SPECTROSCOPY; KINETIC THEORY; MAGNETIC FIELDS; MAGNETIZATION; MAGNETOHYDRODYNAMICS; MATHEMATICAL MODELS; PLASMAS; TURBULENCE;

MAGNETIC ENERGY DENSITY; MAGNETIZED ACCRETION DISC; MAGNETIZED PRESSURE; SHAKURA-SUNYAEV MODEL; THERMAL ENERGY DENSITY;

ASTROPHYSICS;

EID: 0042060952     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20030868     Document Type: Article

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