Shocks in the hottest galaxy clusters produce observable Z/W ratios in the Fe XXV triplet and ion-temperature line broadening that can constrain electron heating and temperature equilibration with XRISM.
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Iron He-triplet signatures of shocks in the hottest galaxy clusters. Z/W line ratio, line broadening, and electron-ion temperature equilibration
Shocks in the hottest galaxy clusters produce observable Z/W ratios in the Fe XXV triplet and ion-temperature line broadening that can constrain electron heating and temperature equilibration with XRISM.