- Abstract:
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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...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Version:
- Accepted Manuscript
- Files:
-
-
(pdf, 9.7MB)
-
- Publisher copy:
- 10.1038/s41550-018-0608-8
-
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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
- Copyright holder:
- McClure-Griffiths et al.
- Copyright date:
- 2018
- Notes:
- © The Author(s) 2018. This is the accepted manuscript version of the article. The final version is available online from Springer Nature at: https://doi.org/10.1038/s41550-018-0608-8
Journal article
Cold gas outflows from the Small Magellanic Cloud traced with ASKAP
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