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We have extracted archival data from the Chandra Data Archive, and the data analysis was supported by the CXC CIAO software and CALDB. We have used the NASA NED and ADS facilities. The computations in this paper were conducted on the Smithsonian High Performance Cluster (SI/HPC). This work was supported by the Chandra GO grants (AR4-15005X and AR5-16007X), by Smithsonian Competitive Grant Program for Science, by Smithsonian 2018 Scholarly Study Program and by NASA contract NAS8- 03060 (CXC).

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