Steady models of optically thin, magnetically supported black hole accretion disks

Publications of the Astronomical Society of Japan

Volumn 59, Issue 2, 2007, Pages 457-465

  Oda, Hiroshi ^a   Machida, Mami ^b   Nakamura, Kenji E ^c   Matsumoto, Ryoji ^a  

^a CHIBA UNIVERSITY   (Japan)

^b NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^c MATSUE NATIONAL COLLEGE OF TECHNOLOGY   (Japan)

Author keywords

Accretion: accretion disks; Black holes; MHD; State transition

Indexed keywords

GRAVITATION; MAGNETOHYDRODYNAMICS; STARS; THERMODYNAMIC STABILITY;

ACCRETION DISCS; ACCRETION RATE; ACCRETION: ACCRETION DISKS; BLACK-HOLE ACCRETION DISCS; MAGNETIC PRESSURE; MAGNETIC-FIELD; STATE TRANSITIONS; STEADY MODEL; STEADY SOLUTION; THERMAL;

BLACK HOLES;

EID: 34250209099     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/59.2.457     Document Type: Article

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