• 责任者：Zhang Qi (Institute of Geology and Geophysics ; Chinese Academy of Sciences ; Beijing 100029 ; China)
• 刊名：Mineral Deposits
• 出版年：2011
• 卷期：30(3)
• 关键词：花岗岩类 ; granitoid ; 金矿 ; gold ores ; 铜矿 ; copper ores ; 钨矿 ; tungsten ores ; 锡矿 ; tin ores
• 页码：p.557-570
• 图表：28 refs.
• 分类号：0801
• issnNo：ISSN0258-7106
• isbnNo：CN11-1965/P

The authors welcome the comments by Hua (2010) and Wang (2010). It is noted that the Sr-Yb classification for granitic rocks that the authors proposed is not the one based on the origin of granitic rocks, instead it is an indicator for the pressure under which the granitic rocks were formed. Therefore, Cu-Au mineralization is associated with adakitic and Himalayan-type granitic rocks formed from thickened lower crust (high-pressure), whereas W-Sn mineralization is related to Nanling-type granitic rocks formed from thinned crust (lower-pressure). The Cu-Au mineralization and the W-Sn mineralization are thus not genetically related to each other; they may be overlapped within the same granitic plutons at different times.oft-com:office:office" />