The role of turbulence in high-mass star formation: Subsonic and transonic turbulence are ubiquitously found at early stages
Artikel i vetenskaplig tidskrift, 2024
Radio lines: ISM
Turbulence
ISM: kinematics and dynamics
Submillimeter: ISM
Stars: formation
Författare
Chao Wang
Beijing University of Technology
Ke Wang
Beijing University of Technology
Feng Wei Xu
Beijing University of Technology
Patricio Sanhueza
The Graduate University for Advanced Studies (SOKENDAI)
National Astronomical Observatory of Japan
Hauyu Baobab Liu
National Sun Yat-Sen University
Qizhou Zhang
Harvard-Smithsonian Center for Astrophysics
Xing Lu
Shanghai Astronomical Observatory
Francesco Fontani
Osservatorio Astrofisico di Arcetri
P. Caselli
Max-Planck-Gesellschaft
Gemma Busquet
Institut d'Estudis Espacials de Catalunya (IEEC)
Universitat de Barcelona
Jonathan Tan
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
Di Li
Chinese Academy of Sciences
Zhejiang Lab
J. M. Jackson
Green Bank Observatory
NASA Ames Research Center
University of Virginia
Thushara Pillai
Boston University
Paul T.P. Ho
Academia Sinica
East Asian Observatory
Andrés E. Guzmán
National Astronomical Observatory of Japan
Nannan Yue
Beijing University of Technology
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 681 A51Ämneskategorier
Astronomi, astrofysik och kosmologi
Strömningsmekanik och akustik
DOI
10.1051/0004-6361/202347024