Stingrays in the radio sky: Two unusual diffuse radio relic sources in the direction of the Magellanic Stream
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arXiv
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| Autori principali: | , , , , , , , , , , , , , , , , , , , |
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| Natura: | Preprint |
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2025
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| author | Smeaton, Zachary J Filipovic, Miroslav D Koribalski, Barbel S Sasaki, Manami Alsaberi, Rami Z E Bradley, Aaron C Crawford, Evan J Dai, Shi Gupta, Nikhel Haberl, Frank Hopkins, Andrew M Jarrett, Thomas H Lazarević, Sanja Leahy, Denis Macgregor, Peter Rowell, Gavin Shabala, Stanislav S Urosevic, Dejan van Loon, Jacco Th Vernstrom, Tessa |
| author_facet | Smeaton, Zachary J Filipovic, Miroslav D Koribalski, Barbel S Sasaki, Manami Alsaberi, Rami Z E Bradley, Aaron C Crawford, Evan J Dai, Shi Gupta, Nikhel Haberl, Frank Hopkins, Andrew M Jarrett, Thomas H Lazarević, Sanja Leahy, Denis Macgregor, Peter Rowell, Gavin Shabala, Stanislav S Urosevic, Dejan van Loon, Jacco Th Vernstrom, Tessa |
| contents | We present the discovery of two extended, low surface brightness radio continuum sources, each consisting of a near-circular body and an extended tail of emission, nicknamed Stingray 1 (ASKAP J0129-5350) and Stingray 2 (ASKAP J0245-5642). Both are found in the direction of the Magellanic Stream (MS) and were discovered in the Australian Square Kilometre Array Pathfinder (ASKAP) Evolutionary Map of the Universe (EMU) survey at 944 MHz. We combine the ASKAP data with low-frequency radio observations from the GaLactic and Extragalactic All-sky MWA Survey (GLEAM) to conduct a radio continuum analysis. We explore both Galactic/near Galactic scenarios, including runaway or circumgalactic supernova remnants (SNRs) and parentless pulsar-wind nebulae (PWNe), and extragalactic scenarios including radio active galactic nuclei (AGNs), dying radio galaxies, galaxy clusters, galaxy pairs or groups, head-tail radio galaxies, and Odd Radio Circles (ORCs), as well as the possibility that the morphology is due to a chance alignment. The Stingrays exhibit non-thermal emission with spectral indices of $α$ = -0.89 $\pm$ 0.09 for Stingray 1 and $α$ = -1.77 $\pm$ 0.06 for Stingray 2. We find that none of the proposed scenarios can explain all of the observed properties, however we determine it most likely that their shape is caused by some kind of complex environmental interaction. The most likely scenario from the available data is that of a head-tail radio galaxy, but more data is required for a definitive classification. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2508_09495 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Stingrays in the radio sky: Two unusual diffuse radio relic sources in the direction of the Magellanic Stream Smeaton, Zachary J Filipovic, Miroslav D Koribalski, Barbel S Sasaki, Manami Alsaberi, Rami Z E Bradley, Aaron C Crawford, Evan J Dai, Shi Gupta, Nikhel Haberl, Frank Hopkins, Andrew M Jarrett, Thomas H Lazarević, Sanja Leahy, Denis Macgregor, Peter Rowell, Gavin Shabala, Stanislav S Urosevic, Dejan van Loon, Jacco Th Vernstrom, Tessa Astrophysics of Galaxies High Energy Astrophysical Phenomena We present the discovery of two extended, low surface brightness radio continuum sources, each consisting of a near-circular body and an extended tail of emission, nicknamed Stingray 1 (ASKAP J0129-5350) and Stingray 2 (ASKAP J0245-5642). Both are found in the direction of the Magellanic Stream (MS) and were discovered in the Australian Square Kilometre Array Pathfinder (ASKAP) Evolutionary Map of the Universe (EMU) survey at 944 MHz. We combine the ASKAP data with low-frequency radio observations from the GaLactic and Extragalactic All-sky MWA Survey (GLEAM) to conduct a radio continuum analysis. We explore both Galactic/near Galactic scenarios, including runaway or circumgalactic supernova remnants (SNRs) and parentless pulsar-wind nebulae (PWNe), and extragalactic scenarios including radio active galactic nuclei (AGNs), dying radio galaxies, galaxy clusters, galaxy pairs or groups, head-tail radio galaxies, and Odd Radio Circles (ORCs), as well as the possibility that the morphology is due to a chance alignment. The Stingrays exhibit non-thermal emission with spectral indices of $α$ = -0.89 $\pm$ 0.09 for Stingray 1 and $α$ = -1.77 $\pm$ 0.06 for Stingray 2. We find that none of the proposed scenarios can explain all of the observed properties, however we determine it most likely that their shape is caused by some kind of complex environmental interaction. The most likely scenario from the available data is that of a head-tail radio galaxy, but more data is required for a definitive classification. |
| title | Stingrays in the radio sky: Two unusual diffuse radio relic sources in the direction of the Magellanic Stream |
| topic | Astrophysics of Galaxies High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2508.09495 |