How do we see a relativistic accretion disk during a thermal instability?

Publications of the Astronomical Society of Japan

Volumn 58, Issue 2, 2006, Pages 477-484

  Kawata, Akihiro ^a   Watarai, Ken Ya ^a,b   Fukue, Jun ^a  

^a OSAKA KYOIKU UNIVERSITY   (Japan)

^b JAPAN SOCIETY FOR THE PROMOTION OF SCIENCE   (Japan)

Author keywords

Accretion, accretion disks; Black holes; Stars: X rays

Indexed keywords

BLACK HOLES; GRAVITATION; PRESSURE; RUPTURE DISKS; STARS;

ACCRETION DISCS; ACCRETION: ACCRETION DISKS; BLACK HOLE CANDIDATES; INCLINATION ANGLES; INNER REGION; PRESSURE-DRIVEN; RADIATION PRESSURE; RELATIVISTICS; STARS: X-RAY; THERMAL INSTABILITIES; X-RAY:STARS;

THERMODYNAMIC STABILITY;

EID: 33646796342     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/58.2.477     Document Type: Article

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