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Variation of the Subhalo Abundance in Dark Matter Halos

  • Authors: Tomoaki Ishiyama, Toshiyuki Fukushige, and Junichiro Makino

ISHIYAMA, FUKUSHIGE, & MAKINO 2009 The Astrophysical Journal 696 2115.

  • Provider: AAS Journals

Caption: Figure 4.

Dependence of the subhalo abundance N >0.10 on ( a) mass M 12 in unit of 10 12M (left), ( b) concentration parameter c = r 0/ R v (right). The white circles denote the halos with 1.5 × 10 12M M < 3 × 10 12M . The black circles denote the halos with 3 × 10 12M M < 1 × 10 13M .

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