A rapidly changing jet orientation in the stellar-mass black-hole system V404 Cygni
- Submitting institution
-
University of Oxford
- Unit of assessment
- 9 - Physics
- Output identifier
- 10534
- Type
- D - Journal article
- DOI
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10.1038/s41586-019-1152-0
- Title of journal
- Nature
- Article number
- -
- First page
- 374
- Volume
- 569
- Issue
- 7756
- ISSN
- 0028-0836
- Open access status
- Exception within 3 months of publication
- Month of publication
- April
- Year of publication
- 2019
- URL
-
-
- Supplementary information
-
-
- Request cross-referral to
- -
- Output has been delayed by COVID-19
- No
- COVID-19 affected output statement
- -
- Forensic science
- No
- Criminology
- No
- Interdisciplinary
- No
- Number of additional authors
-
20
- Research group(s)
-
-
- Citation count
- 27
- Proposed double-weighted
- No
- Reserve for an output with double weighting
- No
- Additional information
- -
- Author contribution statement
- Fender made a major input to the interpretation of the images, to the solutions for jet velocities, angles & powers, and to the discussion of possible connection between the accretion disc and jet angles.
- Non-English
- No
- English abstract
- -