On the weakness of disc models in bright ULXs

Monthly Notices of the Royal Astronomical Society

Volumn 371, Issue 2, 2006, Pages 673-683

  Goncalves A C ^a,b   Soria, R ^c,d  

^a UNIVERSITÉ PARIS DIDEROT   (France)

^b UNIVERSITY OF LISBON   (Portugal)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d UNIVERSITY COLLEGE LONDON   (United Kingdom)

Author keywords

Accretion, accretion discs; Black hole physics; X rays: binaries

Indexed keywords

ABSORPTION SPECTROSCOPY; BLACK HOLES; GRAVITATION; IONIZATION OF GASES;

ACCRETION: ACCRETION DISKS; BLACK HOLE PHYSICS; BLACKBODY COMPONENTS; DISK MODEL; POWER-LAW; POWER-LAW COMPONENTS; SIMPLE++; X RAY SPECTRUM; X-RAY SOURCES; X-RAYS: BINARIES;

STARS;

EID: 33748643207     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.10687.x     Document Type: Article

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