Figure 20.
(a) RGS sepctrum and (b) unabsorbed cooling rate plotted against hidden rate (HCR) for the Perseus cluster after the maximum value of absorbing column density is raised from |$5\times 10^{22}$| to |$10^{23}{{\rm \, cm}^{-2}\, }$|.
(a) RGS sepctrum and (b) unabsorbed cooling rate plotted against hidden rate (HCR) for the Perseus cluster after the maximum value of absorbing column density is raised from |$5\times 10^{22}$| to |$10^{23}{{\rm \, cm}^{-2}\, }$|.
