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Molecular clouds and star formation toward the Galactic plane within 216.25 degrees <= l <= 218.75 degrees and-0.75 degrees. <= b <= 1.25 degrees 期刊论文
ASTRONOMY & ASTROPHYSICS, 2016, 卷号: 588
Authors:  Gong, Y.;  Mao, R. Q.;  Fang, M.;  Zhang, S. B.;  Su, Y.;  Yang, J.;  Jiang, Z. B.;  Xu, Y.;  Wang, M.;  Wang, Y.;  Lu, D. R.;  Sun, J. X.
Adobe PDF(6378Kb)  |  Favorite  |  View/Download:9/0  |  Submit date:2016/09/27
Surveys  Ism: Clouds  Stars: Formation  Radio Lines: Ism  Ism: Kinematics And Dynamics  
Molecular clouds and star formation toward the Galactic plane within 216.25 degrees <= l <= 218.75 degrees and-0.75 degrees. <= b <= 1.25 degrees 期刊论文
ASTRONOMY & ASTROPHYSICS, 2016, 卷号: 588
Authors:  Gong, Y.;  Mao, R. Q.;  Fang, M.;  Zhang, S. B.;  Su, Y.;  Yang, J.;  Jiang, Z. B.;  Xu, Y.;  Wang, M.;  Wang, Y.;  Lu, D. R.;  Sun, J. X.
Favorite  |  View/Download:16/0  |  Submit date:2016/09/27
Surveys  Ism: Clouds  Stars: Formation  Radio Lines: Ism  Ism: Kinematics And Dynamics