The Fundamental Plane Relationship of Astrophysical Black Holes

Details The Fundamental Plane Relationship of Astrophysical Black Holes The Fundamental Plane Relationship of Astrophysical Black Holes

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..373...45w&link_type=abstract

The Central Engine of Active Galactic Nuclei, ASP Conference Series, Vol. 373, proceedings of the conference held 16-21 October,

Physics

Scientific paper

We derived the black hole fundamental plane relationship among the 1.4 GHz radio luminosity (L_r), 0.1-2.4 keV X-ray luminosity (LX), and black hole mass (MBH) from a uniform broad-line SDSS AGN sample. We found in our sample that the fundamental plane relation has a very weak dependence on the black hole mass, and a tight correlation also exists between the Eddington luminosity-scaled X-ray and radio luminosities for the radio-quiet subsample. In addition, we noticed that the radio-quiet and radio-loud AGNs have different power-law slopes in the radio-X-ray nonlinear relationship.

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