Astronomy and Astrophysics – Astrophysics
Scientific paper
2003-04-15
Astrophys.J. 589 (2003) L21-L24
Astronomy and Astrophysics
Astrophysics
Astrophysical Journal Letters, in press
Scientific paper
10.1086/375804
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 sigma^2), with
Hunt Leslie K.
Marconi Alessandro
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