Star formation inside a galactic outflow

R. Maiolino (), H. R. Russell, A. C. Fabian, S. Carniani, R. Gallagher, S. Cazzoli, S. Arribas, F. Belfiore, E. Bellocchi, L. Colina, G. Cresci, W. Ishibashi, A. Marconi, F. Mannucci, E. Oliva and E. Sturm
Additional contact information
R. Maiolino: Cavendish Laboratory, University of Cambridge
H. R. Russell: Institute of Astronomy
A. C. Fabian: Institute of Astronomy
S. Carniani: Cavendish Laboratory, University of Cambridge
R. Gallagher: Cavendish Laboratory, University of Cambridge
S. Cazzoli: CSIC—Departamento de Astrofisica—Centro de Astrobiologia (CSIC-INTA)
S. Arribas: CSIC—Departamento de Astrofisica—Centro de Astrobiologia (CSIC-INTA)
F. Belfiore: Cavendish Laboratory, University of Cambridge
E. Bellocchi: CSIC—Departamento de Astrofisica—Centro de Astrobiologia (CSIC-INTA)
L. Colina: CSIC—Departamento de Astrofisica—Centro de Astrobiologia (CSIC-INTA)
G. Cresci: INAF—Osservatorio Astrofisico di Arcetri
W. Ishibashi: Physik-Institut, Universität Zürich
A. Marconi: INAF—Osservatorio Astrofisico di Arcetri
F. Mannucci: INAF—Osservatorio Astrofisico di Arcetri
E. Oliva: INAF—Osservatorio Astrofisico di Arcetri
E. Sturm: Max-Planck-Institut für Extraterrestrische Physik

Nature, 2017, vol. 544, issue 7649, 202-206

Abstract: Star formation at a rate of more than 15 solar masses a year has been observed inside a massive outflow of gas from a nearby galaxy; this could also be happening inside other galactic outflows.

Date: 2017
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DOI: 10.1038/nature21677

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