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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 12.

Cumulative numbers of subhalos as a function of their maximum rotation velocities V c normalized by the circular velocity of the parent halos at r 50. Three thick solid curves show the average (middle) and ±1σ values (top and bottom). The thick dashed curves show the results of Springel et al. (2008, simulation Aq-A-1, Aq-C-2, Aq-E-2).

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