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A 12.4-day periodicity in a close binary system after a supernova

A 12.4-day periodicity in a close binary system after a supernova

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_swepub_primary_oai_DiVA_org_su_226987

Publication information

Publisher

London: Nature Publishing Group UK

More information

Scope and Contents

Contents

Neutron stars and stellar-mass black holes are the remnants of massive star explosions
1
. Most massive stars reside in close binary systems
2
, and the interplay between the companion star and the newly formed compact object has been theoretically explored
3
, but signatures for binarity or evidence for the formation of a compact...

Alternative Titles

Full title

A 12.4-day periodicity in a close binary system after a supernova

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_swepub_primary_oai_DiVA_org_su_226987

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_swepub_primary_oai_DiVA_org_su_226987

Other Identifiers

ISSN

0028-0836,1476-4687

E-ISSN

1476-4687

DOI

10.1038/s41586-023-06787-x

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