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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 7.

Evolution of the halo half-mass radius R h( t). The solid curves show the results of three subhalo-rich halos. The dashed curves show the results of three subhalo-poor halos. The left panel is for halos with 1.5 × 10 12M M < 2.0 × 10 12M . The right panel is for halos with 2.0 × 10 12M M < 2.5 × 10 12M .

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