Host galaxy morphologies of X-ray selected AGN: Assessing the significance of different black hole fuelling mechanisms to the accretion density of the Universe at z ∼ 1

Monthly Notices of the Royal Astronomical Society

Volumn 397, Issue 2, 2009, Pages 623-633

  Georgakakis, A ^a   Coil, A L ^b   Laird, E S ^c   Griffith, R L ^d   Nandra, K ^c   Lotz, J M ^e   Pierce, C M ^f   Cooper, M C ^g   Newman, J A ^h   Koekemoer, A M ⁱ  

^a NATIONAL OBSERVATORY OF ATHENS   (Greece)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c IMPERIAL COLLEGE LONDON   (United Kingdom)

^d CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^e NATIONAL OPTICAL ASTRONOMY OBSERVATORY   (United States)

^f UNIVERSITY OF CALIFORNIA   (United States)

^g UNIVERSITY OF ARIZONA   (United States)

^h UNIVERSITY OF PITTSBURGH   (United States)

ⁱ STScI   (United States)

Author keywords

Galaxies: evolution; Galaxies: starbursts; Surveys; X rays: galaxies

Indexed keywords

BLACK HOLES; FUELING; GALAXIES; GRAVITATION; LUMINANCE; STARS; STOCHASTIC SYSTEMS;

ACTIVE GALACTIC NUCLEI; BLACK HOLES; DEEP SURVEY; DISK GALAXIES; GALAXIES: STARBURSTS; GALAXY EVOLUTION; HOST GALAXIES; MORPHOLOGICAL INFORMATION; X-RAY OBSERVATIONS; X-RAYS: GALAXIES;

SURVEYS;

EID: 67651089728     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.14951.x     Document Type: Article

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