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Sustained star formation in the central stellar cluster of the Milky Way

Sustained star formation in the central stellar cluster of the Milky Way

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_743475590

Sustained star formation in the central stellar cluster of the Milky Way

About this item

Full title

Sustained star formation in the central stellar cluster of the Milky Way

Author / Creator

Publisher

London: Nature Publishing Group UK

Journal title

Nature (London), 1996-08, Vol.382 (6592), p.602-604

Language

English

Formats

Publication information

Publisher

London: Nature Publishing Group UK

More information

Scope and Contents

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...

Alternative Titles

Full title

Sustained star formation in the central stellar cluster of the Milky Way

Authors, Artists and Contributors

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_miscellaneous_743475590

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_743475590

Other Identifiers

ISSN

0028-0836

E-ISSN

1476-4687

DOI

10.1038/382602a0

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