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Origin of the ring structures in Hercules A

Authors :
R. Timmerman
R. J. van Weeren
J. R. Callingham
W. D. Cotton
R. Perley
L. K. Morabito
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
Galaxies, Etoiles, Physique, Instrumentation (GEPI)
Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
European Commission
European Research Council
Ministerio de Ciencia e Innovación (España)
Source :
Digital.CSIC. Repositorio Institucional del CSIC, instname, Astronomy & astrophysics, 2022, Vol.658, pp.A5 [Peer Reviewed Journal], Astronomy & Astrophysics, 658:A5
Publication Year :
2022

Abstract

This is an 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.<br />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 (<br />R.T. and R.Jv.W. acknowledge support from the ERC Starting Grant ClusterWeb 804208. J.R.C. thanks the Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO) for support via the Talent Programme Veni grant. C.O. and S.B. acknowledge support from the Natural Sciences and Engineering Research Council (NSERC) of Canada. A.B. acknowledges support from the VIDI research programme with project number 639.042.729, which is financed by the Netherlands Organisation for Scientific Research (NWO). J.M. acknowledges financial support from the State Agency for Research of the Spanish MCIU through the “Center of Excellence Severo Ochoa” award to the Instituto de Astrofísica de Andalucía (SEV-2017-0709) and from the grant RTI2018-096228-B-C31 (MICIU/FEDER, EU). This paper is based (in part) on data obtained with the International LOFAR Telescope (ILT) under project code LC14-019. LOFAR (Van Haarlem et al. 2013) is the Low Frequency Array designed and constructed by ASTRON. It has observing, data processing, and data storage facilities in several countries, that are owned by various parties (each with their own funding sources), and that are collectively operated by the ILT foundation under a joint scientific policy. The ILT resources have benefitted from the following recent major funding sources: CNRS-INSU, Observatoire de Paris and Université d’Orléans, France; BMBF, MIWF-NRW, MPG, Germany; Science Foundation Ireland (SFI), Department of Business, Enterprise and Innovation (DBEI), Ireland; NWO, The Netherlands; The Science and Technology Facilities Council, UK; Ministry of Science and Higher Education, Poland. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.

Details

Language :
English
Database :
OpenAIRE
Journal :
Digital.CSIC. Repositorio Institucional del CSIC, instname, Astronomy & astrophysics, 2022, Vol.658, pp.A5 [Peer Reviewed Journal], Astronomy & Astrophysics, 658:A5
Accession number :
edsair.doi.dedup.....8c17e2a28b0d24ab7ce46f014d69e09b