The link between solenoidal turbulence and slow star formation in G0.253+0.016
The link between solenoidal turbulence and slow star formation in G0.253+0.016
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Publisher
Cambridge, UK: Cambridge University Press
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Language
English
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Publisher
Cambridge, UK: Cambridge University Press
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Scope and Contents
Contents
Star formation in the Galactic disc is primarily controlled by gravity, turbulence, and magnetic fields. It is not clear that this also applies to star formation near the Galactic Centre. Here we determine the turbulence and star formation in the CMZ cloud G0.253+0.016. Using maps of 3 mm dust emission and HNCO intensity-weighted velocity obtained...
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Full title
The link between solenoidal turbulence and slow star formation in G0.253+0.016
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Record Identifier
TN_cdi_proquest_miscellaneous_1884114258
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_1884114258
Other Identifiers
ISSN
1743-9213
E-ISSN
1743-9221
DOI
10.1017/S1743921316012357
