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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. 11.

Distribution of mb/mtot in the galactic halo at ﹩z=2.0﹩. The left panel shows mb/mtot against Rh. On the other hand, the right panel shows mb/mtot against the pericentric distance, Rperi. Plus signs in the panels represent each clump. The open circle in the right panel is the clump that is preprocessed by the other halos.

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