tokens: Studies of the evolution of hot gas in elliptical galaxies at UC Santa Cruz were supported during the earlier phases of this work by the NSF and are currently supported by a NASA-funded Chandra Theory Grant for which we are very grateful. F.B. is supported in part by the Prin MIUR grant 2010LY5N2T “The Chemical and Dynamical Evolution of the Milky Way and Local Group Galaxies.”
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