Transient optical emission from a nonstationary accretion disk: A model for optical afterglow of gamma ray bursts

Publications of the Astronomical Society of Japan

Volumn 52, Issue 4, 2000, Pages 711-723

  Lu, Ye ^a,b   Cheng, Kwong Sang ^a   Zhao, Gang ^b  

^a UNIVERSITY OF HONG KONG   (Hong Kong)

^b CHINESE ACADEMY OF SCIENCES   (China)

Author keywords

Accretion disk: Instability; Black holes; Galaxies; Gamma ray bursts; Radiation mechanism

Indexed keywords

BLACK HOLES; DEPOSITION RATES; GAMMA RAYS; THERMODYNAMIC STABILITY; LIGHT EMISSION; ROTATING DISKS;

ACCRETION DISCS; ACCRETION DISK: INSTABILITY; DISK INSTABILITIES; GAMMA RAYS BURSTS; MAIN SEQUENCE STARS; NONSTATIONARY; OPTICAL AFTERGLOW; OPTICAL EMISSIONS; RADIATION MECHANISM; TIME-DEPENDENT BEHAVIOUR;

STARS;

EID: 0034344920     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/52.4.711     Document Type: Article

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