tokens: The authors would like to thank the anonymous referee for helpful comments and suggestions that improved the manuscript. This work is supported in part by NSF grant AST-1412768, NASA ATP grant NNX11AE07G, NASA Chandra grants GO213004B and GO7-18121X, NASA ASTRO-H (Hitomi) Science Support grant NNX16AD55G, the Research Corporation, and by the facilities and staff of the Yale Center for Research Computing. M.G. is supported by NASA through Einstein Postdoctoral Fellowship Award Number PF5-160137 issued by the Chandra X-ray Observatory Center, which is operated by the SAO for and on behalf of NASA under contract NAS8-03060. HPC resources were in part provided by the NASA/Ames HEC Program (SMD-16-7251). FLASH code was in part developed by the DOE NNSA-ASC OASCR Flash center at the University of Chicago. Part of the analysis were performed using the publicly-available yt package (Turk et al. 2011 ).
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