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Cold gas outflows from the Small Magellanic Cloud traced with ASKAP

Abstract:

Feedback from massive stars plays a critical part in the evolution of the Universe by driving powerful outflows from galaxies that enrich the intergalactic medium and regulate star formation1. An important source of outflows may be the most numerous galaxies in the Universe: dwarf galaxies. With small gravitational potential wells, these galaxies easily lose their star-forming material in the presence of intense stellar feedback1,2. Here, we show that a nearby dwarf galaxy—the Small Magellani...

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Publication status:
Published
Peer review status:
Peer reviewed
Version:
Accepted Manuscript

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Publisher copy:
10.1038/s41550-018-0608-8

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Role:
Author
ORCID:
0000-0003-2730-957X
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Role:
Author
ORCID:
0000-0002-9214-8613
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Publisher:
Springer Nature Publisher's website
Journal:
Nature Astronomy Journal website
Volume:
2
Pages:
901–906
Publication date:
2018-10-29
Acceptance date:
2018-09-21
DOI:
EISSN:
2397-3366
Pubs id:
pubs:952336
URN:
uri:7822b680-a0be-45b5-8c9e-c84b97067874
UUID:
uuid:7822b680-a0be-45b5-8c9e-c84b97067874
Local pid:
pubs:952336
Language:
English

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