On the low star formation rate in Saggitarius C
On the low star formation rate in Saggitarius C
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Author / Creator
Publisher
Bristol: IOP Publishing
Journal title
Language
English
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Publisher
Bristol: IOP Publishing
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Scope and Contents
Contents
The Central Molecular Zone (CMZ) contains approximately 10% of the total molecular gas in the Galaxy concentrated in turbulent and dense molecular clouds. The fact that the star formation rate is low in CMZ is an open question, since there is a large amount of dense gas clouds where star formation could have started. Sagittarius (Sgr) C is the only...
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Full title
On the low star formation rate in Saggitarius C
Authors, Artists and Contributors
Author / Creator
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Record Identifier
TN_cdi_proquest_journals_2652902176
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2652902176
Other Identifiers
ISSN
1742-6588
E-ISSN
1742-6596
DOI
10.1088/1742-6596/2238/1/012008
