Magnetic flares in accretion disc coronae and the spectral states of black hole candidates: The case of GX339-4

Monthly Notices of the Royal Astronomical Society

Volumn 304, Issue 4, 1999, Pages 809-820

  Di Matteo, T ^a,c   Celotti, A ^a,b   Fabian, A C ^a  

^a UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^b SISSA   (Italy)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

Accretion, accretion discs; Binaries: general; Magnetic fields; Radiation mechanisms: thermal; Stars: individual: GX339 4

Indexed keywords

BLACK HOLES; BUOYANCY; ENERGY DISSIPATION; GRAVITATION; MAGNETIC FLUX; PHOTONS; STARS; SYNCHROTRON RADIATION;

ACCRETION DISCS; ACCRETION: ACCRETION DISKS; BINARIES:GENERAL; BLACK HOLE CANDIDATES; FLUX TUBES; MAGNETIC FLARES; MAGNETIC-FIELD; RADIATION MECHANISM: THERMAL; STAR: INDIVIDUAL: GX339-4; STARS: INDIVIDUAL: PROXIMA CENTAURI;

MAGNETIC FIELDS;

EID: 0000878989     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1999.02375.x     Document Type: Article

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