Journal article
A rapidly changing jet orientation in the stellar-mass black-hole system V404 Cygni
- Abstract:
-
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 precession1 due to frame-dragging effects that occur when the black-hole spin axis is misaligned with the orbital plane of its companion star2. Recently, theoretical sim...
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- Publication status:
- Published
- Peer review status:
- Peer reviewed
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Authors
Bibliographic Details
- Publisher:
- Nature Research Publisher's website
- Journal:
- Nature Journal website
- Volume:
- 569
- Pages:
- 374-377
- Publication date:
- 2019-05-01
- Acceptance date:
- 2019-02-06
- DOI:
- EISSN:
-
1476-4687
- ISSN:
-
0028-0836
- Pmid:
-
31036949
Item Description
- Language:
- English
- Keywords:
- Subjects:
- Pubs id:
-
996545
- Local pid:
- pubs:996545
- Deposit date:
- 2020-03-12
Terms of use
- Copyright holder:
- Miller-Jones et al.
- Copyright date:
- 2019
- Rights statement:
- © The Author(s), under exclusive licence to Springer Nature Limited 2019
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