Sustained star formation in the central stellar cluster of the Milky Way
Sustained star formation in the central stellar cluster of the Milky Way
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Publisher
London: Nature Publishing Group UK
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Language
English
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Publisher
London: Nature Publishing Group UK
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Contents
THE central stellar bulge of our Galaxy is commonly thought to consist predominantly of a coeval population of very old (~10
10
yr) stars
1–3
. But evidence for young
4
and intermediate-age stars
5,6
in the bulge is accumulating. Here we argue that star formation has been occurring in the molecular gas near the centre of the...
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Full title
Sustained star formation in the central stellar cluster of the Milky Way
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TN_cdi_proquest_miscellaneous_743475590
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_743475590
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ISSN
0028-0836
E-ISSN
1476-4687
DOI
10.1038/382602a0