1703.08183.pdf (1.29 MB)
ALMA observations of cold molecular gas in AGN hosts at z ~ 1.5 – evidence of AGN feedback?
journal contribution
posted on 2023-06-09, 06:31 authored by Mark SargentSimilarly to the cosmic star formation history, the black hole accretion rate density of the Universe peaked at 199% probability of lower depletion time scales and lower molecular gas fractions in AGN hosts with respect to the non-AGN comparison sample. We discuss the implications of these observations on the impact that AGN feedback may have on star formation efficiency of z>1 galaxies.
Funding
From gas to stars: 12 billion years of galaxy growth; G1946-02; Royal Society; LT150041
History
Publication status
- Published
File Version
- Accepted version
Journal
Monthly Notices of the Royal Astronomical SocietyISSN
0035-8711Publisher
Oxford University PressExternal DOI
Issue
4Volume
468Page range
4205-4215Department affiliated with
- Physics and Astronomy Publications
Research groups affiliated with
- Astronomy Centre Publications
Full text available
- Yes
Peer reviewed?
- Yes
Legacy Posted Date
2017-06-06First Open Access (FOA) Date
2017-06-06First Compliant Deposit (FCD) Date
2017-06-05Usage metrics
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