Black Hole Mass estimates in nearby AGN from Host-Bulge Properties

Details Black Hole Mass estimates in nearby AGN from Host-Bulge Properties Black Hole Mass estimates in nearby AGN from Host-Bulge Properties

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008rmxac..32..173b&link_type=abstract

The Nuclear Region, Host Galaxy and Environment of Active Galaxies (Eds. Erika Benítez, Irene Cruz-González, & Yair Krongold) Re

Astronomy and Astrophysics

Astronomy

Galaxies: Active, Galaxies: Interactions

Scientific paper

In this work we present the results of an optical photometric study performed to seven nearby AGN that were selected with the SDSS-DR5 database. Surface photometric techniques have been applied to the data in order to obtain B/D ratio and therefore the M_R(Bulge) magnitudes. Bulge luminosities were then used to estimate the black-hole masse (M_{BH}) in these AGN.

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