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Nonhydrostatic Gas in the Core of the Relaxed Galaxy Cluster A1795

  • Authors: M. Markevitch, A. Vikhlinin, and P. Mazzotta

Markevitch, Vikhlinin, & Mazzotta 2001 The Astrophysical Journal Letters 562 L153.

  • Provider: AAS Journals

Caption: Fig. 3.

Profiles from the northern 60° sector opposite to the edge. (a) Surface brightness. The line shows a fit by a β‐model. (b) Projected temperature profile. The line shows a best‐fit model used to estimate the total mass (Fig. 2e). Errors are 68%.

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