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Massive stars in metal-poor dwarf galaxies are often extreme rotators

Massive stars in metal-poor dwarf galaxies are often extreme rotators

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_3098168559

Massive stars in metal-poor dwarf galaxies are often extreme rotators

About this item

Full title

Massive stars in metal-poor dwarf galaxies are often extreme rotators

Publisher

Cambridge, UK: Cambridge University Press

Journal title

Proceedings of the International Astronomical Union, 2022-05, Vol.18 (S361), p.63-69

Language

English

Formats

Publication information

Publisher

Cambridge, UK: Cambridge University Press

More information

Scope and Contents

Contents

We probe how common extremely rapid rotation is among massive stars in the early universe by measuring the OBe star fraction in nearby metal-poor dwarf galaxies. We apply a new method that uses broad-band photometry to measure the galaxy-wide OBe star fractions in the Magellanic Clouds and three more distant, more metal-poor dwarf galaxies. We find...

Alternative Titles

Full title

Massive stars in metal-poor dwarf galaxies are often extreme rotators

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_3098168559

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_3098168559

Other Identifiers

ISSN

1743-9213

E-ISSN

1743-9221

DOI

10.1017/S1743921322002538

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