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Fig. 7


Mass deposition rate as a function of the temperature from the analysis of the ACIS-I Chandra data of Phoenix within 30 kpc from the center. The AGN emission has been removed (inner 1.5 arcsec). The results have been obtained with a multi-temperature mkcflow plus a mekal model for the hot component. Arrows refer to 1σ upper limits. The shaded area shows the 1σ upper limit based on the analysis of a single-temperature mkcflow model in the 0.33.0 keV temperature range plus a mekal model for the hot component.

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