A Supermassive Black Hole Fundamental Plane for Ellipticals

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Published 2007 June 5 © 2007. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Sudhanshu Barway and Ajit Kembhavi 2007 ApJ 662 L67 DOI 10.1086/519560

1538-4357/662/2/L67

Abstract

We obtain the coefficients of a new fundamental plane for supermassive black holes at the centers of elliptical galaxies, involving measured central black hole mass and photometric parameters that define the light distribution. The galaxies are tightly distributed around this mass fundamental plane, with improvement in the rms residual over those obtained from the MBH-σ and MBH-L relations. This implies a strong multidimensional link between central massive black hole formation and global photometric properties of elliptical galaxies, and provides an improved estimate of black hole mass from galaxy data.

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10.1086/519560