Young massive star cluster formation in the Galactic Centre is driven by global gravitational collapse of high-mass molecular clouds
Ashley T. Barnes(University of Bonn), T. Peters(Max Planck Institute for Astrophysics), J. Alves(University of Vienna), Y. Contreras(Leiden University), J. M. Diederik Kruijssen(Max Planck Society), Adam Ginsburg(European Southern Observatory), John Bally(University of Colorado Boulder), J. Kainulainen(Chalmers University of Technology), Xing Lu(National Astronomical Observatory of Japan), Jonathan D. Henshaw(Max Planck Institute for Astronomy), Laura Gómez(Universidad Nacional Autónoma de México), A. Avison(University of Manchester), J. Ott(National Radio Astronomy Observatory), Cara Battersby(Laboratory for Atmospheric and Space Physics), M. T. Beltrán(Arcetri Astrophysical Observatory), Elisabeth A. C. Mills(National Radio Astronomy Observatory), H. Beuther(Max Planck Institute for Astronomy), Steven N. Longmore(European Southern Observatory), J. M. Rathborne(Commonwealth Scientific and Industrial Research Organisation), G. Garay(University of Chile), Daniel L. Walker(Liverpool John Moores University), J. Mark Jackson(Adelphi Group (United Kingdom))
Cited by 38
Related Papers
The Astropy Project: Building an Open-science Project and Status of the v2.0 Core Package<sup>*</sup>
|The Astronomical Journal|2018|7.3k
CALIFA, the Calar Alto Legacy Integral Field Area survey
|Astronomy and Astrophysics|2011|1.3k
Massive molecular outflows
|Springer Link (Chiba Institute of Technology)|2001|413
The formation and assembly history of the Milky Way revealed by its globular cluster population
|Monthly Notices of the Royal Astronomical Society|2018|365
Variations in the Galactic star formation rate and density thresholds for star formation
|Monthly Notices of the Royal Astronomical Society|2012|352