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On the Fate of the Matter Reinserted within Young Nuclear Stellar Clusters

  • Authors: Filiberto Hueyotl-Zahuantitla, Jan Palouš, Richard Wünsch, Guillermo Tenorio-Tagle, and Sergiy Silich

Hueyotl-Zahuantitla et al. 2013 The Astrophysical Journal 766 92.

  • Provider: AAS Journals

Caption: Figure 6.

Analytic prediction for the centrifugal barrier. The radius R T where mass accumulates as a function of the maximum rotation velocity of star clusters of mass M NSC = 3.3 × 10 8M and central SMBH of mass M SMBH = 10 6M , for different star cluster radius. The squares represent the reference model (model 2) and model 4; see Table 1.

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