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http://dx.doi.org/10.5303/PKAS.2015.30.2.335

SUPER-MASSIVE BLACK HOLE MASS SCALING RELATIONS  

GRAHAM, ALISTER W. (Centre for Astrophysics and Supercomputing, Swinburne University of Technology)
SCOTT, NICHOLAS (Centre for Astrophysics and Supercomputing, Swinburne University of Technology)
SCHOMBERT, JAMES M. (Department of Physics, University of Oregon)
Publication Information
Publications of The Korean Astronomical Society / v.30, no.2, 2015 , pp. 335-339 More about this Journal
Abstract
Using black hole masses which span $10^5-10^{10}M_{\odot}$, the distribution of galaxies in the (host spheroid stellar mass)-(black hole mass) diagram is shown to be strongly bent. While the core-$S{\acute{e}}rsic$ galaxies follow a near-linear relation, having a mean $M_{bh}/M_{sph}$ mass ratio of ~0.5%, the $S{\acute{e}}rsic$ galaxies follow a near-quadratic relation. This is not due to offset pseudobulges, but is instead an expected result arising from the long-known bend in the $M_{sph}{-{\sigma}}$ relation and a log-linear $M_{bh}{-{\sigma}}$ relation.
Keywords
black hole physics; galaxies: bulges; galaxies: fundamental parameters; galaxies: nuclei;
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