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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. 3.

Circular velocity profiles of four randomly selected clumps at ﹩z=2.0﹩. The circular velocities are estimated by ﹩[ GM( < r) / r] ^{1/2}﹩, where r is the distance from the center of the clump and ﹩M( < r) ﹩ is the mass within r. We plot from 0 to 3rsub for r. The upward‐pointing arrows indicate the positions of the rsub values, and the open circles represent the minimum points of the circular profiles.

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