Dynamical Accretion Flows. ALMAGAL: Flows along Filamentary Structures in High-Mass Star-Forming Clusters
M. R. A. Wells,H. Beuther,S. Molinari,P. Schilke,C. Battersby, P. Ho,A. Sanchez-Monge,B. Jones, M. B. Scheuck,J. Syed,C. Gieser,R. Kuiper,D. Elia,A. Coletta,A. Traficante, J. Wallace,A. J. Rigby,R. S. Klessen, Q. Zhang, S. Walch,M. T. Beltran,Y. Tang,G. A. Fuller,D. C. Lis, T. Moeller,F. van der Tak,P. D. Klaassen, S. D. Clarke,L. Moscadelli,C. Mininni, H. Zinnecker,Y. Maruccia,S. Pezzuto,M. Benedettini,J. D. Soler,C. L. Brogan,A. Avison,P. Sanhueza,E. Schisano, T. Liu,F. Fontani,K. L. J. Rygl,F. Wyrowski, J. Bally, D. L. Walker,A. Ahmadi,P. Koch,M. Merello,C. Y. Law,L. Testi ASTRONOMY & ASTROPHYSICS(2024)
关键词
accretion, accretion disks,stars: evolution,stars: massive
AI 理解论文
溯源树
样例
