A persistent ultraviolet outflow from an accreting neutron star binary transient.
Journal
Nature
ISSN: 1476-4687
Titre abrégé: Nature
Pays: England
ID NLM: 0410462
Informations de publication
Date de publication:
Mar 2022
Mar 2022
Historique:
received:
09
07
2021
accepted:
09
12
2021
entrez:
3
3
2022
pubmed:
4
3
2022
medline:
23
4
2022
Statut:
ppublish
Résumé
All disc-accreting astrophysical objects produce powerful disc winds. In compact binaries containing neutron stars or black holes, accretion often takes place during violent outbursts. The main disc wind signatures during these eruptions are blue-shifted X-ray absorption lines, which are preferentially seen in disc-dominated 'soft states'
Identifiants
pubmed: 35236977
doi: 10.1038/s41586-021-04324-2
pii: 10.1038/s41586-021-04324-2
doi:
Types de publication
Journal Article
Langues
eng
Sous-ensembles de citation
IM
Pagination
52-57Informations de copyright
© 2022. The Author(s), under exclusive licence to Springer Nature Limited.
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