“…On the basis of the data from exhumed ultrahigh-pressure (UHP) metamorphic rocks and mantle-derived magmas and xenoliths, the upper crustal fluids are generally considered to be dominated by H 2 O, with subordinate CO 2 , CH 4 , and N 2 , whereas the lower crustal fluids are mostly CO 2 -rich (e.g., Touret, 2009;. The growing importance of CO 2 -rich fluids associated with major orogenic cycles is reinforced by the numerous works in this topic including those of Harlov (2000), Agrad et al (2000), Bakker and Mamtani (2000), Bolder-Schrijver et al (2000), Touret (2001Touret ( , 2009, Tsunogae et al (2002), Mohan et al (2003), Cuney et al (2007), Santosh and Omori (2008) and Santosh and Kusky (2009), among others. Some workers have attempted a combination of mineralogic thermobarometry with microthermometric data of high density carbonic fluid inclusions in anhydrous granulites and charnockites to substantiate the model that CO 2 has been instrumental in the formation and stabilization of the mineral assemblages in these rocks (e.g., Mohan et al, 2003;Santosh and Tsunogae, 2003;Cuney et al, 2007;Santosh et al, 2011;Tsunogae and Santosh, 2011).…”