Title: |
The Close AGN Reference Survey (CARS): Locating the [O III] wing component in luminous local Type 1 AGN |
Authors: |
Singha, M., Husemann, B., Urrutia, T., O'Dea, C. P., Scharwächter, J., Gaspari, M., Combes, F., Nevin, R., Terrazas, B. A., Pérez-Torres, M., Rose, T., Davis, T. A., Tremblay, G. R., Neumann, J., Smirnova-Pinchukova, I., Baum, S. A. |
Source: |
A&A 659, A123 (2022) |
Publication Year: |
2021 |
Collection: |
Astrophysics |
Subject Terms: |
Astrophysics - Astrophysics of Galaxies |
More Details: |
[Abridged]The strong asymmetry in the optical [O III]$\lambda$5007 emission line is one of the best signatures of AGN-driven warm (~10$^4$ K) ionized gas outflows on host galaxy scales. While large spectroscopic surveys like SDSS have characterized the kinematics of [O III] for large samples of AGN, estimating the associated energetics requires spatially resolving these outflows with, for example, IFU studies. As part of CARS we obtained spatially-resolved IFU spectroscopy for a representative sample of 39 luminous type 1 AGN at 0.0180 % of the flux associated with a point-like source. We measure <100 pc offsets in the spatial location of the outflow from the AGN nucleus using the spectro-astrometry technique for these sources. For the other 13 AGN, the [O III] wing emission is resolved and possibly extended on kpc scale. We conclude that [O III] wing emission can be compact or extended in an unbiased luminous AGN sample, where both cases are likely to appear. Electron density in the compact [O III] wing regions (median $n_e$~1900 cm$^{-3}$) is nearly a magnitude higher than in the extended ones (median $n_e$~500 cm$^{-3}$). The presence of spatially extended and compact [O III] wing emission is unrelated to the AGN bolometric luminosity and to inclination effects, which means other features such as time delays, or mechanical feedback/radio jets may shape the ionized gas outflow properties. Comment: Accepted for publication in A&A, 19 pages, 13 figures, 3 tables and appendix, data available at https://cars.aip.de |
Document Type: |
Working Paper |
DOI: |
10.1051/0004-6361/202040122 |
Access URL: |
http://arxiv.org/abs/2111.10418 |
Accession Number: |
edsarx.2111.10418 |
Database: |
arXiv |