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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 8.

( a) Concentration c plotted against the maximum half-mass radius R h,max normalized by the halo virial radius R v (left). ( b) The subhalo abundance N >0.10 plotted against the maximum half-mass radius R h,max normalized by the halo virial radius R v (right). Black circles, white circles, and crosses denote the halos with 2.5 × 10 12M M < 3 × 10 12M , 2.0 × 10 12M M < 2.5 × 10 12M , and 1.5 × 10 12M M < 2.0 × 10 12M , respectively.

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