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Breaking the Law: The M bh-M spheroid Relations for Core-Sérsic and Sérsic Galaxies

  • Authors: Alister W. Graham

Graham 2012 The Astrophysical Journal 746 113.

  • Provider: AAS Journals

Caption: Figure 1.

Optimal M bhM sph and M bh–σ 0 relations for a dozen "core" galaxies (red dots) and a dozen non-barred Sérsic galaxies (blue circles). Blue crosses denote five barred Sérsic galaxies used in Table 1. The dashed lines show the extrapolation of these relations beyond M sph = 7 × 10 10M The dotted lines in the left panel delineate the one-sigma uncertainty on the M bhM sph relation for the Sérsic galaxies. The short lines emanating from the data points show their old location based on the data in Häring & Rix (2004). The faint dot-dashed gray lines in the right panel correspond to a sphere of influence of 0 farcs1 at distances of 3 Mpc (lower) and 6 Mpc (upper), respectively.

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