The evidence against Comptonization as a mechanism to explain the Fe Kα line profile in MCG-6-30-15

Monthly Notices of the Royal Astronomical Society

Volumn 317, Issue 1, 2000, Pages

  Ruszkowski, M ^b   Fabian, A C ^b   Ross, R R ^a   Iwasawa, K ^b  

^a Center for Interdisciplinary Studies   (United States)

^b NONE

Author keywords

Accretion, accretion discs; Black hole physics; Galaxies: active; Galaxies: individual: MCG 6 30 15; Line: profiles

Indexed keywords

BLACK HOLES; GALAXIES; GRAVITATION; RELATIVITY; STARS;

ACCRETION: ACCRETION DISKS; BLACK HOLE PHYSICS; COMPTON; COMPTONIZATION; GALAXIES ACTIVE; GALAXIES: INDIVIDUAL: MCG-6-30-15; KΑ; LINE: PROFILES; RELATIVISTIC EFFECTS; THOMSON;

IRON;

EID: 0002069224     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2000.03789.x     Document Type: Article

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