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    • Sahu, Dipen; Liu, Sheng-Yuan; Liu, Tie; Evans II, Neal J.; Hirano, Naomi; Tatematsu, Ken'ichi; Lee, Chin-Fei; Kim, Kee-Tae; Dutta, Somnath; Alina, Dana; Bronfman, Leonardo; Cunningham, María; Eden, David J.; Garay Brignardello, Guido Alejandro; Goldsmith, Paul F.; He, Jinhua; Hsu, Shih-Ying; Goldsmith, Paul F.; He, Jinhua; Hsu, Shih-Ying; Jhan, Kai-Syun; Johnstone, Doug; Juvela, Mika; Kim, Gwanjeong; Kuan, Yi-Jehng; Kwon, Woojin; Lee, Chang Won; Lee, Jeong-Eun; Li, Di; Li, Pak Shing; Li, Shanghuo; Luo, Qiu-Yi; Montillaud, Julien; Moragha, Anthony; Pelkonen, Veli-Matti; Qin, Sheng-Li; Ristorcelli, Isabelle; Sanhueza, Patricio; Shang, Hsien; Shen, Zhi-Qiang; Soam, Archana; Wu, Yuefang; Zhang, Qizhou; Zhou, Jianjun (IOP, 2021)
      Prestellar cores are self-gravitating dense and cold structures within molecular clouds where future stars are born. They are expected, at the stage of transitioning to the protostellar phase, to harbor centrally concentrated ...
    • Luo, Qiu-yi; Liu, Tie; Tatematsu, Ken'ichi; Liu, Sheng-Yuan; Li, Pak Shing; Di Francesco, James; Johnstone, Doug; Goldsmith, Paul F.; Dutta, Somnath; Hirano, Naomi; Lee, Chin-Fei; Li, Di; Kim, Kee-Tae; Lee, Chang Won; Lee, Jeong-Eun; Liu, Xun-chuan; Juvela, Mika; He, Jinhua; Qin, Sheng-Li; Liu, Hong-Li; Eden, David; Kwon, Woojin; Sahu, Dipen; Li, Shanghuo; Xu, Feng-Wei; Zhang, Si-ju; Hsu, Shih-Ying; Bronfman Aguiló, Leonardo Jaime; Sanhueza, Patricio; Pelkonen, Veli-Matti; Zhou, Jian-wen; Liu, Rong; Gu, Qi-lao; Wu, Yue-fang; Mai, Xiao-feng; Falgarone, Edith; Shen, Zhi-Qiang (IOP, 2022)
      During the transition phase from a prestellar to a protostellar cloud core, one or several protostars can form within a single gas core. The detailed physical processes of this transition, however, remain unclear. We present ...