Image Details
Caption: Fig. 2.
Heating and cooling rate vs. redshift. Dashed lines show heating rate for halo of current mass 1010, 1011, ﹩2\times 10^{12}﹩, ﹩10^{13}﹩, 1014, and 1015 M⊙. Thick solid lines show the cooling rate at the virial radius assuming zero metallicity. Thin solid lines show the cooling rate at the virial radius assuming solar metallicity.
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