Anticorrelation of Variability Amplitude with X-Ray Luminosity for Active Galactic Nuclei

Details Anticorrelation of Variability Amplitude with X-Ray Luminosity for Active Galactic Nuclei Anticorrelation of Variability Amplitude with X-Ray Luminosity for Active Galactic Nuclei

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apj...465..646b&link_type=abstract

Astrophysical Journal v.465, p.646

Astronomy and Astrophysics

Astronomy

19

Galaxies: Active, X-Rays: Galaxies

Scientific paper

The bright-spot model for the short-term X-ray variability of active
galactic nuclei predicts that, statistically, sources with larger
luminosities should have smaller variability amplitudes. This
quantitatively agrees with the analysis of the observational data from
12 high-quality EXOSAT long looks performed by Lawrence & Papadakis.

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