Fig. 12.
ICM cooling rate Ṁcool vs. cavity power Pcav for the sample of clusters from Rafferty et al. (2006). The red data point indicates the Phoenix cluster. The gray dashed line indicates the best power-law fit through the data and is given by log Pcav[1042 erg s−1] = (1.00 ± 0.10) log Ṁcool[M⊙/yr] + (0.45 ± 0.24). All black data points are from Rafferty et al. (2006) and McDonald et al. (2018), and the Phoenix cluster data are from McDonald et al. (2015, 2019).
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