Skip navigation
  • 中文
  • English

DSpace CRIS

  • DSpace logo
  • Home
  • Organizations
  • Researchers
  • Research Outputs
  • Projects
  • Explore by
    • Organizations
    • Researchers
    • Research Outputs
    • Projects
  • Academic & Publications
  • Sign in
  • 中文
  • English
  1. Scholars Hub of the Academia Sinica
  2. Research Outputs

Browsing by Author Gu, Qiusheng


Jump to:
0-9 A B C D E F G H I J K L M N O P Q R S T U V W X Y Z
Showing results 1 to 5 of 5
Issue DateTitleAuthor(s)RelationscopusWOSFulltext/Archive link
2018Filamentary Fragmentation and Accretion in High-mass Star-forming Molecular CloudsLu, Xing; Zhang, Qizhou; Liu, Hauyu Baobab; Sanhueza, Patricio; Tatematsu, Ken’ichi; Feng, Siyi; Smith, Howard A.; Myers, Philip C.; Sridharan, T. K.; Gu, QiushengThe Astrophysical Journal 855(1), 9
2015SMA OBSERVATIONS OF C2H IN HIGH-MASS STAR-FORMING REGIONSJiang, Xue-Jian; Liu, Hauyu Baobab ; Zhang, Qizhou; Wang, Junzhi; Zhang, Zhi-Yu; Li, Juan; Gao, Yu; Gu, QiushengThe Astrophysical Journal 808(2), 114
2019Star Formation Rates of Massive Molecular Clouds in the Central Molecular ZoneLu, Xing; Zhang, Qizhou; Kauffmann, Jens; Pillai, Thushara; Ginsburg, Adam; Mills, Elisabeth A. C.; Diederik, Kruijssen J. M.; Longmore, Steven N.; Battersby, Cara; Liu, Hauyu Baobab ; Gu, QiushengThe Astrophysical Journal 872(2), 171
2017The Molecular Gas Environment in the 20 km s−1Cloud in the Central Molecular ZoneLu, Xing; Zhang, Qizhou; Kauffmann, Jens; Pillai, Thushara; Longmore, Steven N.; Kruijssen, J. M. Diederik; Battersby, Cara; Liu, Hauyu Baobab ; Ginsburg, Adam; Mills, Elisabeth A. C.; Zhang, Zhi-Yu; Gu, QiushengThe Astrophysical Journal 839(1), 1
2014VERY LARGE ARRAY OBSERVATIONS OF AMMONIA IN HIGH-MASS STAR FORMATION REGIONSLu, Xing; Zhang, Qizhou; Liu, Hauyu Baobab ; Wang, Junzhi; Gu, QiushengThe Astrophysical Journal 790(2), 84
Showing results 1 to 5 of 5
Explore by
  • Academic & Publications
  • Organizations
  • Researchers
  • Research Outputs
  • Projects
Build with DSpace-CRIS - Extension maintained and optimized by Logo 4SCIENCE Feedback