An explanation for the soft X-ray excess in active galactic nuclei

Monthly Notices of the Royal Astronomical Society

Volumn 365, Issue 4, 2006, Pages 1067-1081

  Crummy, J ^a   Fabian, A C ^a   Gallo, L ^b   Ross, R R ^c  

^a UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^b MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^c Center for Interdisciplinary Studies   (United States)

Author keywords

Accretion, accretion discs; Galaxies: active; X rays: galaxies

Indexed keywords

BLACK HOLES;

ACCRETION: ACCRETION DISKS; ACTIVE GALACTIC NUCLEI; CONVENTIONAL MODELING; GALAXIES ACTIVE; POWER-LAW; REFLECTION MODELS; SOFT X-RAY; SPECTRA'S; X-RAYS: GALAXIES; XMM-NEWTON;

GALAXIES;

EID: 33645059165     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.09844.x     Document Type: Article

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