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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. 8.

Time evolution of the half‐mass radii of the total, baryon, and dark matter components of the reference clump. Thin solid, dotted, and dashed lines indicate rhlf,tot, rhlf,b, and rhlf,dm, respectively. The thick solid line indicates rsub, which is already shown in Fig. 7.

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