Large turbulent reservoirs of cold molecular gas around high-redshift starburst galaxies

E. Falgarone (), M. A. Zwaan, B. Godard, E. Bergin, R. J. Ivison, P. M. Andreani, F. Bournaud, R. S. Bussmann, D. Elbaz, A. Omont, I. Oteo and F. Walter
Additional contact information
E. Falgarone: LERMA/LRA, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Universités
M. A. Zwaan: European Southern Observatory
B. Godard: LERMA/LRA, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Universités
E. Bergin: University of Michigan
R. J. Ivison: European Southern Observatory
P. M. Andreani: European Southern Observatory
F. Bournaud: CEA/AIM
R. S. Bussmann: Cornell University
D. Elbaz: CEA/AIM
A. Omont: IAP, CNRS, Sorbonne Universités
I. Oteo: European Southern Observatory
F. Walter: Max Planck Institute für Astronomie

Nature, 2017, vol. 548, issue 7668, 430-433

Abstract: Large haloes of diffuse molecular gas discovered around high-redshift starburst galaxies show that galactic feedback, coupled to turbulence and gravity, extends the starburst phase instead of quenching it.

Date: 2017
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DOI: 10.1038/nature23298

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