Kinematics of Galactic Centre clouds shaped by shear-seeded solenoidal turbulence
Artikel i vetenskaplig tidskrift, 2023
Galaxy: centre
stars: formation
ISM: kinematics and dynamics
galaxies: ISM
ISM: evolution
ISM: clouds
Författare
Maya Petkova
Astronomisches Rechen-Institut Heidelberg
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
J. M. D. Kruijssen
Technische Universität München
Coolresearch.io
Jonathan D. Henshaw
Liverpool John Moores University
Max-Planck-Gesellschaft
S. Longmore
Coolresearch.io
Liverpool John Moores University
S. C.O. Glover
Universität Heidelberg
Mattia C. Sormani
Universität Heidelberg
Lucia Armillotta
Princeton University
Ashley T. Barnes
Universität Bonn
R. S. Klessen
Universität Heidelberg
Francisco Nogueras-Lara
European Southern Observatory (ESO)
Robin G. Tress
Observatoire de Sauverny
Jairo Armijos-Abendaño
Escuela Politécnica Nacional
Cardiff University
L. Colzi
Centro de Astrobiologia (CAB)
C. Federrath
Australian National University
Australian Research Council (ARC)
P. J.V. Garcia
Universidad Catolica del Norte
Chinese Academy of Sciences
A. Ginsburg
University of Florida
C. Henkel
King Abdulaziz University
Max-Planck-Gesellschaft
S. Martin
European Southern Observatory Santiago
Atacama Large Millimeter-submillimeter Array (ALMA)
D. Riquelme
Max-Planck-Gesellschaft
Universidad de La Serena
Víctor M. Rivilla
Centro de Astrobiologia (CAB)
Monthly Notices of the Royal Astronomical Society
0035-8711 (ISSN) 1365-2966 (eISSN)
Vol. 525 1 962-968Ämneskategorier
Astronomi, astrofysik och kosmologi
Annan fysik
DOI
10.1093/mnras/stad2344