Astronomy and Astrophysics – Astrophysics
Scientific paper
2006-01-13
New Astron. 11 (2006) 567-576
Astronomy and Astrophysics
Astrophysics
19 pages, 6 figures. Submitted to New Astronomy
Scientific paper
10.1016/j.newast.2006.03.002
The fundamental plane of black hole activity is a non-linear correlation among radio core luminosity, X-ray luminosity and mass of all accreting black holes, both of stellar mass and supermassive, found by Merloni, Heinz and Di Matteo (2003) and, independently, by Falcke, Koerding and Markoff (2004). Here we further examine a number of statistical issues related to this correlation. In particular, we discuss the issue of sample selection and quantify the bias introduced by the effect of distance in two of the correlated quantities. We demonstrate that the fundamental plane relation cannot be a distance artifact, and that its non-linearity must represent an intrinsic characteristic of accreting black holes. We also discuss possible future observational strategies to improve our understanding of this correlation.
Di Matteo Tiziana
Falcke Heino
Heinz Sebastian
Koerding Elmar
Markoff Sera
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