The Relation between Black Hole Mass, Bulge Mass, and Near-Infrared Luminosity

2003/04/15 by Alessandro Marconi, Leslie K. Hunt · 2 citations
Physics and Astronomy · #astro-ph

paper · pdf · doi:10.1086/375804

published as Astrophys.J. 589 (2003) L21-L24 · Astrophysical Journal Letters, in press

arxiv created 2003/04/15 · arxiv updated 2009/12/01

Abstract

We present new accurate near-infrared (NIR) spheroid (bulge) structural parameters obtained by two-dimensional image analysis for all galaxies with a direct black hole (BH) mass determination. As expected, NIR bulge luminosities Lbul and BH masses are tightly correlated, and if we consider only those galaxies with secure BH mass measurement and accurate Lbul (27 objects), the spread of MBH-Lbul is similar to MBH-sigma, where sigma is the effective stellar velocity dispersion. We find an intrinsic rms scatter of ~0.3 dex in log MBH. By combining the bulge effective radii R_e measured in our analysis with sigma, we find a tight linear correlation (rms ~ 0.25 dex) between MBH and the virial bulge mass (propto R_e sigma²), with <MBH/Mbul> ~ 0.002. A partial correlation analysis shows that MBH depends on both sigma and R_e, and that both variables are necessary to drive the correlations between MBH and other bulge properties.

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