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Lookup NU author(s): Dr Chris HarrisonORCiD
This is the final published version of an article that has been published in its final definitive form by Oxford University Press, 2021.
For re-use rights please refer to the publisher's terms and conditions.
© 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.We present results from a polarization study of the radio-intermediate quasar, III Zw 2, at a redshift of 0.089, with the upgraded Giant Metrewave Radio Telescope (uGMRT) at 685 MHz and the Karl G. Jansky Very Large Array (VLA) at 5 and 34 GHz. We detect a kpc-scale outflow, exhibiting transverse magnetic (B-) fields. The curved jet terminates in a bow-shock-like radio structure with inferred B-fields aligned with the lobe edges. We suggest that the radio outflow in III Zw 2 is a combination of a collimated jet along with a wind-like component. This 'wind' component could be a magnetized accretion disc wind or the outer layers of a broadened jet or a combination of both. The current data cannot differentiate between these possibilities. We also detect kpc-scale lobe emission that is misaligned with the primary lobes in the uGMRT images. The spectral indices and the electron lifetimes in the misaligned lobe are similar to the primary lobe, suggesting that the misaligned lobe is not a relic. We propose that changing spectral states of the accretion disc, and the subsequent intermittent behaviour of the outflow, along with the close interplay between the jet and 'wind' could explain the radio-intermediate nature of III Zw 2. Our study shows that radio-intermediate quasars are promising sources for understanding the role of jets and winds in galaxy evolution and demonstrates the power of radio polarization studies towards achieving this.
Author(s): Silpa S, Kharb P, Harrison CM, Ho LC, Jarvis ME, Ishwara-Chandra CH, Sebastian B
Publication type: Article
Publication status: Published
Journal: Monthly Notices of the Royal Astronomical Society
Year: 2021
Volume: 507
Issue: 1
Pages: 991-1001
Print publication date: 01/10/2021
Online publication date: 20/08/2021
Acceptance date: 20/06/2021
Date deposited: 14/08/2024
ISSN (print): 0035-8711
ISSN (electronic): 1365-2966
Publisher: Oxford University Press
URL: https://doi.org/10.1093/mnras/stab1870
DOI: 10.1093/mnras/stab1870
Data Access Statement: The data underlying this article will be shared on reasonable request to the corresponding author. The VLA data underlying this article can be obtained from the NRAO Science Data Archive (https://archive.nrao.edu/archive/advquery.jsp) using the proposal ids: 20A-182, 17A-027, and 15A-070. The GMRT data underlying this article can be obtained from the GMRT Online Archive (https://naps.ncra.tifr.res.in/goa/data/search) using the proposal id: DDTC130. The HST data underlying this article can be obtained from the MAST HST Archive (https://archive.stsci.edu/hst/search.php) using the proposal id: ICNO01010.
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