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The Luminosity Dependence of the Galaxy Merger Rate

  • Authors: D. R. Patton and J. E. Atfield

Patton & Atfield 2008 The Astrophysical Journal 685 235.

  • Provider: AAS Journals

Caption: Fig. 3.

﹩N_{c}﹩ plotted vs. absolute magnitude for SDSS, for pairs in five ranges of projected separation. Over the range ﹩-22< M_{r}< -18﹩, the mean ﹩N_{c}﹩ for close pairs (5–20 ﹩h^{-1}﹩ kpc) is ﹩0.021\pm 0.001﹩. The ﹩N_{c}﹩ distribution is approximately flat for the smallest separation pairs, and becomes steeper as pair separation increases.

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