1999
DOI: 10.1007/bf02886165
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Two granitic plutons in Central Western Kunlun Belt: Their ages and possible sources

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Cited by 18 publications
(8 citation statements)
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“…Both of them are formed during the Triassic, and are related to the closure of the Paleo-Tethys ocean basin. Moreover, island-type and collision-type granites with the ages of 180-225 Ma, outcropping in the central (in the southern Kudi, Mazha, and Sanshiliyingfang) and the eastern (in the southern Kangxiwar) Kangxiwar tectonic zone [16,[34][35][36][37][38][39][40] lend further support for the cognition that the Kangxiwar tectonic zone was formed in the Indosinian.…”
Section: Tectonic Significancementioning
confidence: 84%
“…Both of them are formed during the Triassic, and are related to the closure of the Paleo-Tethys ocean basin. Moreover, island-type and collision-type granites with the ages of 180-225 Ma, outcropping in the central (in the southern Kudi, Mazha, and Sanshiliyingfang) and the eastern (in the southern Kangxiwar) Kangxiwar tectonic zone [16,[34][35][36][37][38][39][40] lend further support for the cognition that the Kangxiwar tectonic zone was formed in the Indosinian.…”
Section: Tectonic Significancementioning
confidence: 84%
“…1a) (e.g. Jiang et al 2001Jiang et al , 2002Jiang et al , 2013Xiao et al 2005;Xu et al 1992Xu et al , 1996Yuan et al 1999Yuan et al , 2002Wang et al 2013). The Early Mesozoic granitoids, located in the Southern Kunlun and Taxkogan-Tianshuihai terranes along the Mazar-Kangxiwar faults, occupy a specific position during the Eurasia-Tethys tectonic evolution in this area.…”
Section: Regional Geologymentioning
confidence: 96%
“…1), which provides excellent exposures of interlayered mafic, hybrid, and felsic magmatic rocks. We combine detailed field relationships, zircon U-Pb-Hf iso topic data, whole-rock geochemistry, and thermodynamic modeling to elucidate the processes through which the pluton was constructed and evolved 404 Ma (Yuan et al, 1999) 441±5 Ma (Cui et al, 2006) 447±7 Ma (Cui et al, 2006) 443±2 Ma (Cui et al, 2006) 502±9 Ma (Cui et al, 2006) 500±1 Ma (Cui et al, 2006) 468±3 Ma (Cui et al, 2006) 507±10 Ma (Zhang et al, 2007) 320-331 Ma (Zhang et al, 2006;Kang et al, 2015) 408 Ma (Xiao et al, 2005) 441±2 Ma (Wang et al, 2013) 430-460 Ma (Li et al, 2007;Ye et al, 2008; this study) 471±5 Ma (Yuan et al, 2003) 431±3 Ma (Cui et al, 2006) 456±7 Ma (Feng et al, 2014) 446-449 Ma (Yu et al, 2011) 430±1 Ma (Yang et al, 2016) 440-470 Ma (Gao et al, 2013) 500-514 Ma (Zhang et al, 2016) 515±2 Ma (Zhu et al, 2016) 530±6 Ma (Zhu et al, 2016) 440-480 Ma (Zheng et al, 2013) Fig. 1C L o n g m u c u o F a u l t 531±3 Ma (Yin et al, 2020) 525-533 Ma (Liu et al, 2019) 38 driven by intruded mafic magmas.…”
Section: ■ Introductionmentioning
confidence: 99%