A recurrent nova super-remnant in the Andromeda galaxy
- Submitting institution
-
The University of Manchester
- Unit of assessment
- 9 - Physics
- Output identifier
- 85176759
- Type
- D - Journal article
- DOI
-
10.1038/s41586-018-0825-4
- Title of journal
- Nature
- Article number
- -
- First page
- 460
- Volume
- 565
- Issue
- 7740
- ISSN
- 1476-4687
- Open access status
- Deposit exception
- Month of publication
- January
- 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
-
17
- Research group(s)
-
A - Physics & Astro
- Citation count
- 7
- Proposed double-weighted
- No
- Reserve for an output with double weighting
- No
- Additional information
- -
- Author contribution statement
- Timothy O'Brien: O’Brien was responsible for much of the hydrodynamics simulation work using code he helped develop with his students over years, the version in this case with N. M. H. Vaytet, who is also on the author list. These simulations are essential to the paper as they underpin the main claim which is that a recurrent nova can explain the presence of a “super-remnant”. O’Brien’s contribution forms the basis of the results displayed in Figure 3 of the paper. O’Brien contributed to the discussion, proposing and planning of observations, data interpretation and writing of this manuscript.
- Non-English
- No
- English abstract
- -
