“…Such enrichment is also known for granitoid rocks affected by exchange with meteoric water and/or brines of seawater origin (e.g., Wenner and Taylor, 1976;Harper et al, 1995;Beyth et al, 1997). Igneous rocks with δ 18 O WR values lower than +6‰ can either form through the assimilation of a low-18 O protolith into the magma chamber (e.g., Bacon et al, 1989;Gilliam and Valley, 1997;Balsley and Gregory, 1998;Bindeman and Valley, 2000;Zheng et al, 2004) or by post-magmatic alteration at higher temperatures (generally >300 °C) (e.g., Taylor, 1971Taylor, , 1974Taylor, , 1977Larson and Taylor, 1986). The δD WR values for the majority of igneous rocks fall in the range of -85 to -50‰ (e.g., Taylor, 1974Taylor, , 1977.…”