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Mass Distribution in Galaxy Cluster Cores

  • Authors: M. T. Hogan, B. R. McNamara, F. Pulido, P. E. J. Nulsen, H. R. Russell, A. N. Vantyghem, A. C. Edge, and R. A. Main

2017 The Astrophysical Journal 837 51.

  • Provider: AAS Journals

Caption: Figure 1.

Projected temperature, density, cooling time (tcool), and entropy profiles. The dotted horizontal lines in panels (c) and (d) show the thresholds for cooling time of 5 × 108 yr and for entropy of 30 keV cm2, respectively. Note that all sources satisfy both thresholds (see Section 3.1). Regardless of this and unlike the other four sources shown here, A2029 does not display nebular emission indicative of ongoing cooling.

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