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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 4.

Column densities as seen from the central SMBH for the reference model. The thick solid red line displays the total column density along each line of sight. The thin solid magenta line shows the column density for hot gas, T ⩾3 × 10 5 K. The thin-dotted blue line represents the column density for warm phase, 1500 K < T <3 × 10 5 K. The column densities of cold matter ( T ⩽ 1500 K) are shown by thick-dotted green lines. The cold gas does not cover all the sky.

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