A dense 0.1-solar-mass star in a 51-minute-orbital-period eclipsing binary. (2022)
Attributed to:
A consolidated grant for Sheffield Astrophysics 2021-2024
funded by
STFC
Abstract
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Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1038/s41586-022-05195-x
PubMed Identifier: 36198793
Publication URI: http://europepmc.org/abstract/MED/36198793
Type: Journal Article/Review
Volume: 610
Parent Publication: Nature
Issue: 7932
ISSN: 0028-0836