Spence, R.A.W. orcid.org/0000-0002-2678-4101, Tadhunter, C.N., Rose, M. et al. (1 more author) (2018) Quantifying the AGN-driven outflows in ULIRGs (QUADROS) III: Measurements of the radii and kinetic powers of 8 near-nuclear outflows. Monthly Notices of the Royal Astronomical Society, 478 (2). pp. 2438-2460. ISSN 0035-8711
Abstract
As part of the Quantifying ULIRG AGN-driven Outflows (QUADROS) project to quantify the impact of active galactic nuclei (AGN)-driven outflows in rapidly evolving galaxies in the local Universe, we present observations of eight nearby ultraluminous infrared galaxies (ULIRGs, 0.04 < z < 0.2) taken with the Intermediate-dispersion Spectrograph and Imaging System on the William Herschel Telescope (WHT), and also summarize the results of the project as a whole. Consistent with Rose et al. (2018), we find that the outflow regions are compact (0.08 < R[O III] < 1.5 kpc), and the electron densities measured using the [S II], [O II] trans-auroral emission-line ratios are relatively high (2.5 < log ne (cm−3) < 4.5, median log ne (cm−3) ∼ 3.1). Many of the outflow regions are also significantly reddened (median E(B − V) ∼ 0.5). Assuming that the deprojected outflow velocities are represented by the fifth percentile velocities (v05) of the broad, blueshifted components of [O III] λ5007, we calculate relatively modest mass outflow rates (0.1 < M < ˙ 20 M yr−1, median M˙ ∼ 2 M yr−1), and find kinetic powers as a fraction of the AGN bolometric luminosity (F˙ = E/L ˙ bol) in the range 0.02 < F <˙ 3 per cent (median F˙ ∼ 0.3 per cent). The latter estimates are in line with the predictions of multi-stage outflow models, or single-stage models in which only a modest fraction of the initial kinetic power of the inner disc winds is transferred to the larger scale outflows. Considering the QUADROS sample as a whole, we find no clear evidence for correlations between the properties of the outflows and the bolometric luminosities of the AGN, albeit based on a sample that covers a relatively small range in Lbol. Overall, our results suggest that there is a significant intrinsic scatter in outflow properties of ULIRGs for a given AGN luminosity
Metadata
Item Type: | Article |
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Authors/Creators: |
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Copyright, Publisher and Additional Information: | This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2018 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. |
Keywords: | galaxies: active; galaxies: evolution; galaxies: kinematics and dynamics |
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/M001350/1 |
Depositing User: | Symplectic Sheffield |
Date Deposited: | 25 Jun 2018 14:24 |
Last Modified: | 25 Jun 2018 14:24 |
Published Version: | https://doi.org/10.1093/mnras/sty1046 |
Status: | Published |
Publisher: | Oxford University Press |
Refereed: | Yes |
Identification Number: | 10.1093/mnras/sty1046 |
Related URLs: | |
Open Archives Initiative ID (OAI ID): | oai:eprints.whiterose.ac.uk:132485 |