Black hole feedback in the luminous quasar PDS 456
- Submitting institution
-
University of Keele
- Unit of assessment
- 9 - Physics
- Output identifier
- 289
- Type
- D - Journal article
- DOI
-
10.1126/science.1259202
- Title of journal
- Science
- Article number
- -
- First page
- 860
- Volume
- 347
- Issue
- 6224
- ISSN
- 0036-8075
- Open access status
- Out of scope for open access requirements
- Month of publication
- February
- Year of publication
- 2015
- URL
-
https://science.sciencemag.org/content/347/6224/860.full
- 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
-
19
- Research group(s)
-
-
- Citation count
- 130
- Proposed double-weighted
- No
- Reserve for an output with double weighting
- No
- Additional information
- This paper presented the discovery of fast (0.25c) P Cygni wind profiles measured in the XMM-Newton observations of the quasar, PDS 456 and demonstrated its impact for mechanical feedback into the host galaxy. Dr Reeves was the Principal Investigator of the large XMM-Newton program which was presented in the paper and assumed overall leadership of the project. First-author Nardini was Reeves's post-doc at the time; as first and second authors, Drs Nardini and Reeves contributed equally to both the analysis of the XMM-Newton data and in writing the paper for Science.
- Author contribution statement
- -
- Non-English
- No
- English abstract
- -
