ATOMS: ALMA Three-millimeter Observations of massive Star-forming regions – XX. Probability distribution function of integrated intensity for dense molecular gas tracers
【刊名】Monthly Notices of the Royal Astronomical Society
【作者单位】1Department of Physics, Taiyuan Normal University , Jinzhong 030619 , China;2Institute of Computational and Applied Physics, Taiyuan Normal University , Jinzhong 030619 , China;3Shanghai Astronomical Observatory, Chinese Academy of Sciences , 80 Nandan Road, Shanghai 200030 , China;4National Astronomical Observatories, Chinese Academy of Sciences , Beijing 100012 , P. R. China;5Research Center for Astronomical Computing, Zhejiang Laboratory , Hangzhou 311100 , China;6Department of Astronomy, Yunnan University , Kunming 650091 , P. R. China;7Kavli Institute for Astronomy and Astrophysics, Peking University , 5 Yiheyuan Road, Haidian District, Beijing 100871 , P. R. China;8National Astonomical Observatories, Chinese Academy of Sciences , A20 Datun Road, Chaoyang District, Beijing 100101 , China;9Department of Astronomy, Tsinghua University , Beijing 100084 , China;10Chinese Academy of Sciences South America Center for Astronomy, National Astronomical Observatories, CAS , Beijing 100101 , China;11Instituto de Astronomía, Universidad Católica del Norte , Avenida Angamos 0610, Antofagasta , Chile;12Departamento de Astronomí a, Universidad de Chile , Casilla 36-D, 8320168 Santiago , Chile;13Department of Physics, University of Helsinki , PO Box 64, FI-00014 Helsinki , Finland;14Korea Astronomy and Space Science Institute , 776 Daedeokdaero, Yuseong-gu, Daejeon 34055 , Republic of Korea;15University of Science and Technology, Korea (UST) , 217 Gajeong-ro, Yuseong-gu, Daejeon 34113 , Republic of Korea;16Physikalisches Institut, Universität zu Köln , Zülpicher Straße 77, D-50937 Köln , Germany;17Kavli Institute for Astronomy and Astrophysics, Peking University , Beijing 100871 , P. R. China;18Department of Astronomy, School of Physics, Peking University , Beijing 100871 , P. R. China;19Institute of Physics and Astronomy, Eotvos Lorand University , Pazmany Peter setany 1/A, H-1117 Budapest , Hungary;20University of Debrecen, Institute of Physics , Bem tér 1, H-4032 Debrecen , Hungary;21Institute of Theoretical Astrophysics, University of Oslo, Sem Sælands vei 13 , 0371 Oslo , Norway;22Department of Earth and Planetary Sciences, Institute of Science Tokyo , Meguro, Tokyo 152-8551 , Japan;23National Astronomical Observatory of Japan, National Institutes of Natural Sciences , 2-21-1 Osawa, Mitaka, Tokyo 181-8588 , Japan
【年份】2025
【卷号】Vol.538 No.1
【页码】1-10
【ISSN】0035-8711
【关键词】stars: formation ISM: clouds
【摘要】 We report the observations of J = 1–0 of HCN, HCO|$^+$|, H|$^{13}$|CO|$^{+}$|, and H|$^{13}$|CN, HC|$_3$|N emission towards 135 massive star-forming clumps, as part of the ALMA Three-millimeter Observations of Massive Star-forming regions Survey. ...
