Browsing by Author "Luo, Qiuyi"
Now showing items 1-3 of 3
-
Jhan, Kai-Syun; Lee, Chin-Fei; Johnstone, Doug; Liu, Tie; Liu, Sheng-Yuan; Hirano, Naomi; Tatematsu, Ken'ichi; Dutta, Somnath; Moraghan, Anthony; Shang, Hsein; Lee, Jeong-Eun; Li, Shanghuo; Liu, Chun-Fan; Hsu, Shih-Ying; Kwon, Woojin; Sahu, Dipen; Liu, Xun-Chuan; Kim, Kee-Tae; Luo, Qiuyi; Qin, Sheng-Li; Sanhueza, Patricio; Bronfman Aguiló, Leonardo Jaime; Qizhou, Zhang; Eden, David; Traficante, Alessio; Lee, Chang Won (IOP, 2022)We have selected six sources (G209.55-19.68S2, G205.46-14.56S1(-)A, G203.21-11.20W2, G191.90-11.21S, G205.46-14.56S3, and G206.93-16.61W2) from the Atacama Large Millimeter/submillimeter Array Survey of Orion Planck Galactic ...
-
Dutta, Somnath; Lee, Chin-Fei; Johnstone, Doug; Liu, Tie; Hirano, Naomi; Liu, Sheng-Yuan; Lee, Jeong-Eun; Shang, Hsien; Tatematsu, Ken'ichi; Kim, Kee-Tae; Sahu, Dipen; Sanhueza, Patricio; Di Francesco, James; Jhan, Kai-Syun; Lee, Chang Won; Kwon, Woojin; Li, Shanghuo; Bronfman Aguiló, Leonardo Jaime; Liu, Hong-li; Traficante, Alessio; Kuan, Yi-Jehng; Hsu, Shih-Ying; Moraghan, Anthony; Liu, Chun-Fan; Eden, David; Soam, Archana; Luo, Qiuyi (IOP, 2022)Jets and outflows trace the accretion history of protostars. High-velocity molecular jets have been observed from several protostars in the early Class 0 phase of star formation, detected with the high-density tracer SiO. ...
-
Dutta, Somnath; Lee, Chin-Fei; Hirano, Naomi; Liu, Tie; Johnstone, Doug; Liu, Sheng-Yuan; Tatematsu, Ken'ichi; Goldsmith, Paul F.; Sahu, Dipen; Evans, Neal J.; Sanhueza, Patricio; Kwon, Woojin; Qin, Sheng-Li; Samal, Manash Ranjan; Zhang, Qizhou; Kim, Kee-Tae; Shang, Hsien; Lee, Chang Won; Moraghan, Anthony; Jhan, Kai-Syun; Li, Shanghuo; Lee, Jeong-Eun; Traficante, Alessio; Juvela, Mika; Bronfman Aguiló, Leonardo Jaime; Eden, David; Soam, Archana; He, Jinhua; Liu, Hong-li; Kuan, Yi-Jehng; Pelkonen, Veli-Matti; Luo, Qiuyi; Yi, Hee-Weon; Hsu, Shih-Ying (IOP, 2022)Protostellar outflows and jets play a vital role in star formation as they carry away excess angular momentum from the inner disk surface, allowing the material to be transferred toward the central protostar. Theoretically, ...