A rapidly changing jet orientation in the stellar-mass black-hole system V404 Cygni.
Journal
Nature
ISSN: 1476-4687
Titre abrégé: Nature
Pays: England
ID NLM: 0410462
Informations de publication
Date de publication:
05 2019
05 2019
Historique:
received:
29
08
2018
accepted:
06
02
2019
pubmed:
1
5
2019
medline:
1
5
2019
entrez:
1
5
2019
Statut:
ppublish
Résumé
Powerful relativistic jets are one of the main ways in which accreting black holes provide kinetic feedback to their surroundings. Jets launched from or redirected by the accretion flow that powers them are expected to be affected by the dynamics of the flow, which for accreting stellar-mass black holes has shown evidence for precession
Identifiants
pubmed: 31036949
doi: 10.1038/s41586-019-1152-0
pii: 10.1038/s41586-019-1152-0
doi:
Types de publication
Journal Article
Research Support, U.S. Gov't, Non-P.H.S.
Research Support, Non-U.S. Gov't
Langues
eng
Sous-ensembles de citation
IM
Pagination
374-377Références
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