Scholtz, J., Harrison, C.M., Rosario, D.J. et al. (7 more authors) (2021) The impact of ionised outflows from z∼2.5 quasars is not through instantaneous in-situ quenching: the evidence from ALMA and VLT/SINFONI. Monthly Notices of the Royal Astronomical Society, 505 (4). pp. 5469-5487. ISSN 0035-8711
Abstract
We present high-resolution (∼2.4 kpc) ALMA band 7 observations (rest-frame λ ∼ 250μm) of three powerful z∼2.5 quasars (Lbol = 1047.3-1047.5 ergs s−1). These targets have previously been reported as showing evidence for suppressed star formation based on cavities in the narrow Hα emission at the location of outflows traced with [O III] emission. Here we combine the ALMA observations with a re-analysis of the VLT/SINFONI data to map the rest-frame far-infrared emission, Hα emission, and [O III] emission. In all targets we observe high velocity [O III] gas (i.e. W80 ∼ 1000–2000 km s−1) across the whole galaxy. We do not identify any Hα emission that is free from contamination from AGN-related processes; however, based on SED analyses, we show that the ALMA data contains a significant dust-obscured star formation component in two out of the three systems. This dust emission is found to be extended over ≈1.5–5.5 kpc in the nuclear regions, overlaps with the previously reported Hα cavities and is co-spatial with the peak in surface brightness of the [O III] outflows. In summary, within the resolution and sensitivity limits of the data, we do not see any evidence for a instantaneous shut down of in-situ star formation caused directly by the outflows. However, similar to the conclusions of previous studies and based on our measured star formation rates, we do not rule out that the global host galaxy star formation could be suppressed on longer timescales by the cumulative effect of quasar episodes during the growth of these massive black holes.
Metadata
Item Type: | Article |
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Authors/Creators: |
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Copyright, Publisher and Additional Information: | © 2021 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. This is an author-produced version of a paper subsequently published in Monthly Notices of the Royal Astronomical Society. Uploaded in accordance with the publisher's self-archiving policy. |
Keywords: | galaxies: active; galaxies: evolution; X-rays: galaxies; infrared: galaxies |
Dates: |
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Institution: | The University of Sheffield |
Academic Units: | The University of Sheffield > Faculty of Science (Sheffield) > Department of Physics and Astronomy (Sheffield) |
Funding Information: | Funder Grant number SCIENCE AND TECHNOLOGY FACILITIES COUNCIL ST/R000964/1 |
Depositing User: | Symplectic Sheffield |
Date Deposited: | 25 Jun 2021 08:48 |
Last Modified: | 25 Feb 2022 18:37 |
Status: | Published |
Publisher: | Oxford University Press (OUP) |
Refereed: | Yes |
Identification Number: | 10.1093/mnras/stab1631 |
Open Archives Initiative ID (OAI ID): | oai:eprints.whiterose.ac.uk:175593 |