The Correlation between Supermassive Black Hole Mass and the Structure of Ellipticals and Bulges
We demonstrate a strong correlation between supermassive black hole (SMBH) mass and the global structure of ellipticals and bulges: more centrally concentrated bulges and ellipticals (higher Sérsic index n) host higher-mass black holes. This correlation is as good as that previously found between SMBH mass and central velocity dispersion, with
Erwin, P. et al.
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2004