Now showing items 1-5 of 5

    • 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. ...
    • 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 ...
    • Tatematsu, Ken'Ichi; Liu, Tie; Ohashi, Satoshi; Sanhueza, Patricio; Nguyen Lu'O'Ng, Quang; Hirota, Tomoya; Liu, Sheng Yuan; Hirano, Naomi; Choi, Minho; Kang, Miju; Thompson, Mark A.; Fuller, Gary; Wu, Yuefang; Li, Di; Di Francesco, James; Kim, Kee Tae; Wang, Ke; Ristorcelli, Isabelle; Juvela, Mika; Shinnaga, Hiroko; Cunningham, María; Saito, Masao; Lee, Jeong-Eun; Tóth, L. Viktor; He, Jinhua; Sakai, Takeshi; Kim, Jungha (IOP Publishing, 2017)
      We observed 13 Planck cold clumps with the James Clerk Maxwell Telescope/SCUBA-2 and with the Nobeyama 45 m radio telescope. The N2H+ distribution obtained with the Nobeyama telescope is quite similar to SCUBA-2 dust ...
    • Evans II, Neal J.; Di Francesco, James; Lee, Jeong-Eun; Jørgensen, Jes K.; Choi, Minho; Myers, Philip C.; Mardones Pérez, Diego (The American Astronomical Society, 2015)
      Observations of the isolated globule B335 with ALMA have yielded absorption features against the continuum that are redshifted from the systemic velocity in both HCN and HCO+ lines. These features provide unambiguous ...
    • Tatematsu, Ken'ichi; Kim, Gwanjeong; Liu, Tie; Evans, Neal J.; Yi, Hee-Weon; Lee, Jeong-Eun; Wu, Yuefang; Hirano, Naomi; Liu, Sheng-Yuan; Dutta, Somnath; Sahu, Dipen; Sanhueza, Patricio; Kim, Kee-Tae; Juvela, Mika; Toth, L. Viktor; Feher, Orsolya; He, Jinhua; Ge, Jixing; Feng, Siyi; Choi, Minho; Kang, Miju; Thompson, Mark A.; Fuller, Gary A.; Li, Di; Ristorcelli, Isabelle; Wang, Ke; Di Francesco, James; Eden, David; Ohashi, Satoshi; Nguyen Lu'o'ng, Quang; Shinnaga, Hiroko; Kim, Jungha (IOP, 2021)
      We present the results of on-the-fly mapping observations of 44 fields containing 107 SCUBA-2 cores in the emission lines of molecules N2H+, HC3N, and CCS at 82-94 GHz using the Nobeyama 45 m telescope. This study aimed ...