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

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

Young massive clusters (YMCs) are the most compact, high-mass stellar systems still forming at the present day. The precursor clouds to such systems are, however, rare due to their large initial gas mass reservoirs and rapid dispersal time-scales due to stellar feedback. None the less, unlike their high-z counterparts, these precursors are resolvable down to the sites of individually forming stars, and hence represent the ideal environments in which to test the current theories of star and cluster formation. Using high angular resolution (1 arcsec / 0.05 pc) and sensitivity ALMA observations of two YMC progenitor clouds in the Galactic Centre, we have identified a suite of molecular line transitions - e.g. c-C3H2 (7 - 6) - that are believed to be optically thin, and reliably trace the gas structure in the highest density gas on star-forming core scales. We conduct a virial analysis of the identified core and proto-cluster regions, and show that half of the cores (5/10) and both proto-clusters are unstable to gravitational collapse. This is the first kinematic evidence of global gravitational collapse in YMC precursor clouds at such an early evolutionary stage. The implications are that if these clouds are to form YMCs, then they likely do so via the 'conveyor-belt' mode, whereby stars continually form within dispersed dense gas cores as the cloud undergoes global gravitational collapse. The concurrent contraction of both the cluster-scale gas and embedded (proto-)stars ultimately leads to the high (proto-)stellar density in YMCs.

Organisation(s)
Department of Astrophysics
External organisation(s)
Liverpool John Moores University (LJMU), Max-Planck-Institut für extraterrestrische Physik, Rheinische Friedrich-Wilhelms-Universität Bonn, Atacama Large Millimetre Array (ALMA), University of Manchester, Leiden University, National Radio Astronomy Observatory, Socorro, Max-Planck-Institut für Astronomie, Commonwealth Scientific and Industrial Research Organisation (CSIRO), Joint ALMA Observatory, National Astronomical Observatory of Japan, University of Colorado, Boulder, University of Connecticut, INAF - Osservatorio Astrofisico di Arcetri, Universidad de Chile, NASA Ames Research Center, Chalmers University of Technology, Ruprecht-Karls-Universität Heidelberg, Brandeis University, Max-Planck-Institut für Astrophysik
Journal
Monthly Notices of the Royal Astronomical Society
Volume
486
Pages
283-303
ISSN
0035-8711
DOI
https://doi.org/10.1093/mnras/stz796
Publication date
06-2019
Peer reviewed
Yes
Austrian Fields of Science 2012
103003 Astronomy, 103004 Astrophysics
Keywords
Portal url
https://ucris.univie.ac.at/portal/en/publications/young-massive-star-cluster-formation-in-the-galactic-centre-is-driven-by-global-gravitational-collapse-of-highmass-molecular-clouds(3d862b48-4c36-4db9-a242-bb95cae277a8).html