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Bright radio emission from an ultraluminous stellar-mass microquasar in M 31

Bright radio emission from an ultraluminous stellar-mass microquasar in M 31

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_swepub_primary_oai_DiVA_org_su_87696

Publication information

Publisher

London: Nature Publishing Group UK

More information

Scope and Contents

Contents

A new ultraluminous X-ray source has been discovered in M 31, whose variability and associated bright, compact radio emission identify it as a stellar-mass black hole accreting close to the Eddington limit.
The ULX factor in the Andromeda galaxy
Ultra-luminous X-ray sources, or ULXs, are a subject of controversy as their extreme luminosities...

Alternative Titles

Full title

Bright radio emission from an ultraluminous stellar-mass microquasar in M 31

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_swepub_primary_oai_DiVA_org_su_87696

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_swepub_primary_oai_DiVA_org_su_87696

Other Identifiers

ISSN

0028-0836,1476-4687

E-ISSN

1476-4687

DOI

10.1038/nature11697

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