【作者】C Zhang，Feng-Yao Zhu，Tie Liu，Z-Y Ren，H-L Liu，Ke Wang，J-W Wu，Y Zhang，J-W Zhou，K Tatematsu，Guido Garay，Anandmayee Tej，Shanghuo Li，W F Xu，Chang Won Lee，Leonardo Bronfman，Archana Soam，D Li
【刊名】Monthly Notices of the Royal Astronomical Society
【作者单位】1Department of Physics, Taiyuan Normal University, Jinzhong 030619, China;Institute of Computational and Applied Physics, Taiyuan Normal University, Jinzhong 030619, China;zhangchao920610@126.com 2Research Center for Intelligent Computing Platforms, Zhejiang Laboratory, Hangzhou 311100, China;zhufya@icloud.com 3Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, China;liutie@shao.ac.cn 4National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, P.R. China 5Department of Astronomy, Yunnan University, Kunming 650091, P.R., China 6Kavli Institute for Astronomy and Astrophysics, Peking University, 5 Yiheyuan Road, Haidian District, Beijing 100871, P.R., China 7National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, P.R. China;University of Chinese Academy of Sciences, Beijing 100049, P.R., China 8School of Physics and Astronomy, Sun Yat-sen University, 2 Daxue Road, Zhuhai, Guangdong 519082, P.R. China 9Nobeyama Radio Observatory, National Astronomical Observatory of Japan, National Institutes of Natural Sciences, Nobeyama, Minamimaki, Minamisaku, Nagano 384-1305, Japan 10Departamento de Astronomia, Universidad de Chile, Las Condes, Santiago 3659, Chile 11Indian Institute of Space Science and Technology, Thiruvananthapuram 695 547, Kerala, India 12Max Planck Institute of Astronoy, Königstuhl 17, Heidelberg 69117, Germany;SOFIA Science Centre, USRA, NASA Ames Research Centre, MS-12, N232, Moffett Field, CA 94035, USA 13Korea Astronomy and Space Science Institute, 776 Daedeokdaero, Yuseong-gu, Daejeon 34055, Republic of Korea;University of Science and Technology, 217 Gajeong-ro Yuseong-gu, Daejeon 34113, Republic of Korea 14SOFIA Science Centre, USRA, NASA Ames Research Centre, MS-12, N232, Moffett Field, CA 94035, USA 15National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, P.R. China;NAOC-UKZN Computational Astrophysics Centre, University of KwaZulu-Natal, Durban 4000, South Africa
【年份】2022
【卷号】Vol.520 No.3
【页码】3245-3258
【ISSN】0035-8711
【摘要】 Hydrogen radio recombination lines are one of the major diagnostics of the physical properties of H II regions. We use RRL H40α, He40α, and 3 mm continuum emission to investigate the properties of a large sample of resolved UC H II regions identifie...
