The relationship between X-ray variability amplitude and black hole mass in active galactic nuclei

Monthly Notices of the Royal Astronomical Society

Volumn 358, Issue 4, 2005, Pages 1405-1416

  O'Neill, Paul M ^a   Nandra, Kirpal ^a   Papadakis, Iossif E ^b   Turner, T J ^c,d  

^a IMPERIAL COLLEGE LONDON   (United Kingdom)

^b UNIVERSITY OF CRETE   (Greece)

^c NASA GODDARD SPACE FLIGHT CENTER   (United States)

^d UNIVERSITY OF MARYLAND BALTIMORE COUNTY   (United States)

Author keywords

Galaxies: active; Galaxies: nuclei; Galaxies: Seyfert; X rays: galaxies

Indexed keywords

BLACK HOLES; GALAXIES; GRAVITATION; LUMINANCE; STARS; STOCHASTIC SYSTEMS; UNCERTAINTY ANALYSIS;

ACTIVE GALACTIC NUCLEI; ANTICORRELATION; BLACK HOLE MASS; GALAXIES ACTIVE; GALAXIES:NUCLEI; GALAXY:SEYFERT; TIME-SCALES; UNCERTAINTY; X-RAY VARIABILITY; X-RAYS: GALAXIES;

POWER SPECTRUM;

EID: 17744365020     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.08860.x     Document Type: Article

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