【作者】C Zhang，Neal J Evans，T Liu，J-W Wu，Ke Wang，H-L Liu，F-Y Zhu，Z-Y Ren，L K Dewangan，Chang Won Lee，Shanghuo Li，L Bronfman，A Tej，D Li
【刊名】Monthly Notices of the Royal Astronomical Society
【作者单位】1 Department of Physics, Taiyuan Normal University , Jinzhong 030619, China; 2 Institute of Computational and Applied Physics, Taiyuan Normal University , Jinzhong 030619, China; 3 Department of Astronomy, The University of Texas at Austin , 2515 Speedway, Stop C1400, Austin, TX 78712-1205, USA; 4 Shanghai Astronomical Observatory, Chinese Academy of Sciences , 80 Nandan Road, Shanghai 200030, China; 5 University of Chinese Academy of Sciences, School of Astronomy and Space Science , Beijing 100049, China; 6 National Astronomical Observatories, Chinese Academy of Sciences , Beijing 100012, China; 7 Kavli Institute for Astronomy and Astrophysics, Peking University , 5 Yiheyuan Road, Haidian District, Beijing 100871, China; 8 Department of Astronomy, Yunnan University , Kunming 650091, China; 9 Physical Research Laboratory , Navrangpura, Ahmedabad 380009, Gujarat, India; 10 Korea Astronomy and Space Science Institute , 776 Daedeokdaero, Yuseong-gu, Daejeon 34055, Republic of Korea; 11 University of Science and Technology , Korea, 217 Gajeong-ro, Yuseong-gu, Daejeon 34113, Republic of Korea; 12 Departamento de Astronomía, Universidad de Chile , Casilla 36-D, 8320168, Santiago, Chile; 13 Indian Institute of Space Science and Technology , Thiruvananthapuram 695547, Kerala, India; 14 NAOC–UKZN Computational Astrophysics Centre, University of KwaZulu-Natal , Durban 4000, South Africa
【年份】2022
【卷号】Vol.510 No.4
【页码】4998-5008
【ISSN】0035-8711
【关键词】stars: formation ISM: clouds H ii regions radio lines: ISM
【摘要】 We report the detection of radio recombination line H 40α towards 75 sources, with data obtained from ACA observations in the ATOMS survey of 146 active Galactic star-forming regions. We calculated ionized gas mass and star formation rate with H...
