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Galaxy Growth by Merging in the Nearby Universe

  • Authors: Tao Jiang, David W. Hogg, and Michael R. Blanton

Jiang, Hogg, & Blanton 2012 The Astrophysical Journal 759 140.

  • Provider: AAS Journals

Caption: Figure 9.

Relationship between σ v , the stellar velocity dispersion and M, the stellar mass for red galaxies in the spectroscopic sample. The gray scale and the contours reflect the number of galaxies in each bin. The solid line is the linear fit, Equation (6).

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