AGN wind scaling relations and the co-evolution of black holes and galaxies
- Submitting institution
-
University of Southampton
- Unit of assessment
- 9 - Physics
- Output identifier
- 34061332
- Type
- D - Journal article
- DOI
-
10.1051/0004-6361/201629478
- Title of journal
- Astronomy & Astrophysics
- Article number
- A143
- First page
- 1
- Volume
- 601
- Issue
- -
- ISSN
- 0004-6361
- Open access status
- Compliant
- Month of publication
- May
- Year of publication
- 2017
- 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
-
16
- Research group(s)
-
-
- Citation count
- 173
- Proposed double-weighted
- No
- Reserve for an output with double weighting
- No
- Additional information
- -
- Author contribution statement
- As the title suggests, this project relies on two parts intimately connected. The first one, more observational, deals with the “AGN wind scaling relations”, and the second one, more theoretical, dealing with the “co-evolution of black holes and galaxies”. Shankar led the latter part, devising the continuity equation models to compute the mean accretion rates of black holes in a cosmological context. Shankar, together with the first author and the co-author, defined a novel methodology to connect the observational part to the theoretical part to constrain AGN winds.
- Non-English
- No
- English abstract
- -
