| Download | - View final version: MeerKAT 1.3 GHz observations of supernova remnants (PDF, 12.9 MiB)
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| DOI | Resolve DOI: https://doi.org/10.3847/1538-4365/ad0ecb |
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| Author | Search for: Cotton, W. D.ORCID identifier: https://orcid.org/0000-0001-7363-6489; Search for: Kothes, R.1ORCID identifier: https://orcid.org/0000-0001-5953-0100; Search for: Camilo, F.ORCID identifier: https://orcid.org/0000-0002-1873-3718; Search for: Chandra, P.ORCID identifier: https://orcid.org/0000-0002-0844-6563; Search for: Buchner, S.; Search for: Nyamai, M.ORCID identifier: https://orcid.org/0000-0002-8973-4072 |
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| Affiliation | - National Research Council of Canada. Herzberg Astronomy and Astrophysics
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| Format | Text, Article |
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| Subject | supernova remnants |
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| Abstract | We present full Stokes MeerKAT L-band (856–1712 MHz) observations of 36 high-latitude supernova remnants (SNRs). Sensitive, high-dynamic-range images show a wealth of structure. G15.1−1.6 appears to be a H ii region rather than an SNR. G30.7−2.0 consists of three background extragalactic sources which appear to form an arc when imaged with much lower resolution. At least half of the remnants in the sample contain "blowouts" or "ears," showing these to be a common feature. Analysis of the polarimetric data reveals details of the magnetic field structure in the emitting regions of the remnants as well as magnetized thermal plasma in front of polarized emission. The chance alignment of G327.6+14.6 with a background active galactic nucleus with very extended polarized jets allows testing for the presence of Faraday effects in the interior of the remnant. Scant evidence of Faraday rotating material is found in the interior of this remnant. |
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| Publication date | 2024-01-18 |
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| Publisher | IOP |
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| Licence | |
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| Language | English |
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| Peer reviewed | Yes |
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| Export citation | Export as RIS |
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| Report a correction | Report a correction (opens in a new tab) |
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| Record identifier | c601fef2-64a5-4114-af50-93d87ec25878 |
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| Record created | 2024-06-10 |
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| Record modified | 2024-06-10 |
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