The relation between the mid-infrared emission and Black Hole Mass in Active Galactic Nuclei: A direct way to probe black hole growth?

Details The relation between the mid-infrared emission and Black Hole Mass in Active Galactic Nuclei: A direct way to probe black hole growth? The relation between the mid-infrared emission and Black Hole Mass in Active Galactic Nuclei: A direct way to probe black hole growth?

2002-04-16

arxiv.org/abs/astro-ph/0204269v1

Astronomy and Astrophysics

Astrophysics

Accepted for publication in the Astrophysical Journal Letters

Scientific paper

10.1086/341198

We use a large, heterogeneous sample of local active galactic nuclei (AGN) that includes Seyfert 1s, Seyfert 2s and PG quasars to investigate for the first time the relation between black hole mass (M_BH) and mid-infrared nuclear emission. We find a clear relation between M_BH and the 10 micron nuclear luminosity for these local AGNs. There are no significant differences between type 1 and type 2 objects, implying that the reprocessing of the 10 micron nuclear emission is not severely affected by geometric and optical depth effects. We also confirm that M_BH is related to the 2-10keV X-ray luminosity, but only for the Compton thin galaxies. We present a theoretical basis for these empirical relations and discuss possible reasons for the observed scatter. Our results show that rest-frame 10 micron and hard X-ray luminosities (especially the former, which is applicable to all AGN types) can be powerful tools for conducting a census of black hole masses at high redshift and for probing their cosmological evolution.

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