EMU detection of mysterious multiple component radio-continuum emission from nearby spiral Seyfert I type galaxy ‘Sand-timer’ (NGC 7213)

We present an Australian Square Kilometre Array Pathfinder (ASKAP) Evolutionary Map of the Universe (EMU) radio-continuum detection of the nearby spiral Seyfert I type galaxy NGC 7213 which we nickname ‘sand-timer’ due to its morphological appearance. We find an intriguing and peculiar emission extending from the central supermassive black hole (SMBH), which we refer to as galaxy hyperbubbles and/or active galactic nucleus (AGN) jets. Finally, we find two previously undetected kiloparsec-scale features in the polarised intensity image, which appear most likely also related to the central SMBH, as restarted bipolar radio jets, though somewhat obscured in the radio-continuum total intensity image. They resemble the bow shocks often seen in Fanaroff-Riley Class II (FR-II) radio galaxies, and so we propose they most likely represent an early episode of the ‘Sand-timer’s’ AGN jet activity. An alternative scenario is that the core of NGC 7213 may be a super massive binary black hole (SMBBH) which is undergoing a tidal disruption event (TDE), potentially causing the peculiar radio-continuum emission.

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Journal
The Open Journal of Astrophysics
Published
2026-10-15
DOI
https://doi.org/10.33232/001c.172532
Primary Topic
Astrophysical Phenomena and Observations
Type
article
Field-Weighted Citation Impact
0.00

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article

EMU detection of mysterious multiple component radio-continuum emission from nearby spiral Seyfert I type galaxy ‘Sand-timer’ (NGC 7213)

R. Kothes, E. Järvelä, N. F. H. Tothill, D. Leahy et al.
The Open Journal of Astrophysics
Astrophysical Phenomena and Observations
article

EMU detection of mysterious multiple component radio-continuum emission from nearby spiral Seyfert I type galaxy ‘Sand-timer’ (NGC 7213)

R. Kothes, E. Järvelä, N. F. H. Tothill, D. Leahy, Zachary J. Smeaton, J. Th. van Loon, S. Shabala, E. J. Crawford, S. F. ur Rahman, M. Selby, B. S. Koribalski, A. C. Bradley, R. Z. E. Alsaberi, G. L. White, G. P. Rowell, A. Ahmad, M. D. Filipović, E. J. Stanton, D. Urosević, V. Velović, H. Sano, S. Taziaux, J. L. Payne, A. M. Hopkins, S. Lazarević, C. Bordiu, K. Tsuge
article en

Abstract

We present an Australian Square Kilometre Array Pathfinder (ASKAP) Evolutionary Map of the Universe (EMU) radio-continuum detection of the nearby spiral Seyfert I type galaxy NGC 7213 which we nickname ‘sand-timer’ due to its morphological appearance. We find an intriguing and peculiar emission extending from the central supermassive black hole (SMBH), which we refer to as galaxy hyperbubbles and/or active galactic nucleus (AGN) jets. Finally, we find two previously undetected kiloparsec-scale features in the polarised intensity image, which appear most likely also related to the central SMBH, as restarted bipolar radio jets, though somewhat obscured in the radio-continuum total intensity image. They resemble the bow shocks often seen in Fanaroff-Riley Class II (FR-II) radio galaxies, and so we propose they most likely represent an early episode of the ‘Sand-timer’s’ AGN jet activity. An alternative scenario is that the core of NGC 7213 may be a super massive binary black hole (SMBBH) which is undergoing a tidal disruption event (TDE), potentially causing the peculiar radio-continuum emission.

The Open Journal of AstrophysicsVol. 9
Texas Tech University (US), University of Tasmania (AU), Australia Telescope National Facility (AU), University of Calgary (CA), University of Karachi (PK), Dominion Astrophysical Observatory (CA), University of Belgrade (RS), Osservatorio Astrofisico di Catania (IT), Gifu University (JP), Keele University (GB), The University of Adelaide (AU), Western Sydney University (AU), National Institute for Astrophysics (IT), Ruhr University Bochum (DE), Macquarie University (AU)
Science and Industry Endowment Fund, Astronomy Australia Limited, Australian Government, Commonwealth Scientific and Industrial Research Organisation, Curtin University of Technology, Bulgarian Academy of Sciences, Government of Western Australia, Serbian Academy of Sciences and Arts
Openalex Percentile: Top 15%
Astrophysical Phenomena and Observations
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