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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 1.

Number of subhalos of S1 plotted against those of S2. Here, N x, i, Sj is the number of subhalos for halo i with normalized rotation velocity larger than x, in simulation S j. Open circles, squares and triangles show N >0.15, N >0.10 and N >0.05, respectively.

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