Fig. 7 from Tidal Disruption of Dark Matter Halos around Proto

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Tidal Disruption of Dark Matter Halos around Proto–Globular Clusters

Authors: Takayuki R. Saitoh, Jin Koda, Takashi Okamoto, Keiichi Wada, and Asao Habe

Saitoh et al. 2006 The Astrophysical Journal 640 22.

Provider: AAS Journals

Caption: Fig. 7.

Time evolution of the size of the reference clump (r_sub) and tidal radius (r_tidal). The thick solid line and dashed line indicate r_sub and r_tidal, respectively. The distance of the clump from the galactic center is shown by the thin solid line (see Fig. 6). The dotted line indicates R_h before capture of the host galactic halo.

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