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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. 12.

Distribution of mb/mtot against Rperi/Rapo in the galactic halo at ﹩z=2.0﹩. Red, blue, orange, and purple numbers indicate different ranges of the pericentric distance from ﹩1< R_{\mathrm{peri}\,}/ \mathrm{kpc}\,< 2﹩ to ﹩4< R_{\mathrm{peri}\,}/ \mathrm{kpc}\,< 5﹩, and the numbers indicate how many times each clump passes the pericenter. We obtain pericenters and apocenters from the most recent period of the clumps. Note that we do not consider clumps that have never passed pericenters or larger pericentric distances ﹩R_{\mathrm{peri}\,}> 5﹩ kpc in this plot.

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