R. Timmerman
Origin of the ring structures in Hercules A. Sub-arcsecond 144 MHz to 7 GHz observations
Timmerman, R.; van Weeren, R.J.; Callingham, J.R.; Cotton, W.D.; Perley, R.; Morabito, L.K.; Gizani, N.A.B.; Bridle, A.H.; O'Dea, C.P.; Baum, S.A.; Tremblay, G.R.; Kharb, P.; Kassim, N.E.; Röttgering, H.J.A.; Botteon, A.; Sweijen, F.; Tasse, C.; Brüggen, M.; Moldon, J.; Shimwell, T.; Brunetti, G.
Authors
R.J. van Weeren
J.R. Callingham
W.D. Cotton
R. Perley
Professor Leah Morabito leah.k.morabito@durham.ac.uk
Professor
N.A.B. Gizani
A.H. Bridle
C.P. O'Dea
S.A. Baum
G.R. Tremblay
P. Kharb
N.E. Kassim
H.J.A. Röttgering
A. Botteon
F. Sweijen
C. Tasse
M. Brüggen
J. Moldon
T. Shimwell
G. Brunetti
Abstract
The prominent radio source Hercules A features complex structures in its radio lobes. Although it is one of the most comprehensively studied sources in the radio sky, the origin of the ring structures in the Hercules A radio lobes remains an open question. We present the first sub-arcsecond angular resolution images at low frequencies (<300 MHz) of Hercules A, made with the International LOFAR Telescope. With the addition of data from the Karl G. Jansky Very Large Array, we mapped the structure of the lobes from 144 MHz to 7 GHz. We explore the origin of the rings within the lobes of Hercules A, and test whether their properties are best described by a shock model, where shock waves are produced by the jet propagating in the radio lobe, or by an inner-lobe model, where the rings are formed by decelerated jetted plasma. From spectral index mapping our large frequency coverage reveals that the curvature of the different ring spectra increases with distance away from the central active galactic nucleus. We demonstrate that the spectral shape of the rings is consistent with synchrotron aging, which speaks in favor of an inner-lobe model where the rings are formed from the deposition of material from past periods of intermittent core activity.
Citation
Timmerman, R., van Weeren, R., Callingham, J., Cotton, W., Perley, R., Morabito, L., Gizani, N., Bridle, A., O'Dea, C., Baum, S., Tremblay, G., Kharb, P., Kassim, N., Röttgering, H., Botteon, A., Sweijen, F., Tasse, C., Brüggen, M., Moldon, J., Shimwell, T., & Brunetti, G. (2022). Origin of the ring structures in Hercules A. Sub-arcsecond 144 MHz to 7 GHz observations. Astronomy & Astrophysics, 658, Article A5. https://doi.org/10.1051/0004-6361/202140880
Journal Article Type | Article |
---|---|
Acceptance Date | Jul 1, 2021 |
Online Publication Date | Jan 25, 2022 |
Publication Date | 2022-02 |
Deposit Date | Oct 5, 2021 |
Publicly Available Date | Oct 22, 2021 |
Journal | Astronomy and astrophysics. |
Print ISSN | 0004-6361 |
Electronic ISSN | 1432-0746 |
Publisher | EDP Sciences |
Peer Reviewed | Peer Reviewed |
Volume | 658 |
Article Number | A5 |
DOI | https://doi.org/10.1051/0004-6361/202140880 |
Public URL | https://durham-repository.worktribe.com/output/1237647 |
Files
Published Journal Article
(6.2 Mb)
PDF
Publisher Licence URL
http://creativecommons.org/licenses/by/4.0/
Published Journal Article
(6.3 Mb)
PDF
Copyright Statement
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
You might also like
LOFAR HBA observations of the Euclid Deep Field North (EDFN)
(2024)
Journal Article
Cosmic evolution of FRI and FRII sources out to z = 2.5
(2024)
Journal Article
Downloadable Citations
About Durham Research Online (DRO)
Administrator e-mail: dro.admin@durham.ac.uk
This application uses the following open-source libraries:
SheetJS Community Edition
Apache License Version 2.0 (http://www.apache.org/licenses/)
PDF.js
Apache License Version 2.0 (http://www.apache.org/licenses/)
Font Awesome
SIL OFL 1.1 (http://scripts.sil.org/OFL)
MIT License (http://opensource.org/licenses/mit-license.html)
CC BY 3.0 ( http://creativecommons.org/licenses/by/3.0/)
Powered by Worktribe © 2024
Advanced Search