Young massive star cluster formation in the Galactic Centre is driven by global gravitational collapse of high-mass molecular clouds

Author(s):: Barnes, A.T.; Longmore, S.N.; Avison, A.; Contreras Morales, Y.A. (0000-0002-6388-3635); Ginsburg, A.; Henshaw, J.D.; Rathborne, J.M.; Walker, D.L.; Alves, J.; Bally, J.; Battersby, C.; Beltrán, M.T.; Beuther, H.; Garay, G.; Gomez, L.; Jackson, J.; Kainulainen, J.; Kruijssen, J.M.D.; Lu, X.; Mills, E.A.C.; Ott, J.; Peters, T.

Published: 2019
Publication type: Article / Letter to editor

Date issued: 2019-03-19
Language: English
Is part of: Monthly Notices of the RAS (0035-8711) (2019), Vol. 486, no. 1, p. 283-303
hdl: 1887/84767
doi: 10.1093/mnras/stz796
URL: https://ui.adsabs.harvard.edu/abs/2019MNRAS.486..283B