The XBS sample of type 1 AGNs: Radio loudness vs. physical parameters

Details The XBS sample of type 1 AGNs: Radio loudness vs. physical parameters The XBS sample of type 1 AGNs: Radio loudness vs. physical parameters

2009-09-23

arxiv.org/abs/0909.4165v1

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

2 pages, 2 figures, to appear on the proceedings of the conference "Accretion and Ejection in AGN: A Global View", June 22-26

Scientific paper

We have studied the relationship between the AGN radio-loudness and the mass
of the central black-hole by using the ~190 type 1 AGN selected in the
XMM-Newton Bright Survey (XBS). We find that radio-loud AGNs are much more
frequent at high black-hole masses being a factor ~10 times more common for
masses >10^9 Msun when compared to masses between 10^7-10^9 Msun.

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