Detection of Diffuse Radio Emission inside the Supernova Remnant G338.3-0.0 associated with the Gamma-ray Source HESS J1640-465
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arXiv
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| Format: | Preprint |
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2025
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| _version_ | 1866909753378078720 |
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| author | Abdelmaguid, Moaz Gelfand, Joseph Alford, Jason |
| author_facet | Abdelmaguid, Moaz Gelfand, Joseph Alford, Jason |
| contents | We report the discovery of diffuse radio emission within SNR G338.3-0.0 using new MeerKAT observations at 816 MHz and 1.4 GHz. The radio emission spatially overlaps with the X-ray pulsar wind nebula (PWN) powered by PSR J1640-4631 and the GeV/TeV gamma-ray source HESS J1640-465. The morphology of this radio emission is centrally peaked and its extent is well-contained within the SNR shell. A lack of mid- and far-infrared counterparts and the absence of catalogued H II regions argues against a thermal origin, while the morphology and radial profile are suggestive of a PWN origin powered by PSR J1640-4631. Under this assumption, we use a one-zone, time dependant model to reproduce the size and broadband (radio, X-ray, and gamma-rays) spectral energy distribution of the PWN. The modelling and broadband properties of this PWN suggests it is currently interacting with the reverse shock within its host SNR. This evolutionary stage is associated with particles escaping the PWN and entering the ISM, suggesting this object may be an important source of Galactic PeV e+/e- |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2508_18999 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Detection of Diffuse Radio Emission inside the Supernova Remnant G338.3-0.0 associated with the Gamma-ray Source HESS J1640-465 Abdelmaguid, Moaz Gelfand, Joseph Alford, Jason High Energy Astrophysical Phenomena We report the discovery of diffuse radio emission within SNR G338.3-0.0 using new MeerKAT observations at 816 MHz and 1.4 GHz. The radio emission spatially overlaps with the X-ray pulsar wind nebula (PWN) powered by PSR J1640-4631 and the GeV/TeV gamma-ray source HESS J1640-465. The morphology of this radio emission is centrally peaked and its extent is well-contained within the SNR shell. A lack of mid- and far-infrared counterparts and the absence of catalogued H II regions argues against a thermal origin, while the morphology and radial profile are suggestive of a PWN origin powered by PSR J1640-4631. Under this assumption, we use a one-zone, time dependant model to reproduce the size and broadband (radio, X-ray, and gamma-rays) spectral energy distribution of the PWN. The modelling and broadband properties of this PWN suggests it is currently interacting with the reverse shock within its host SNR. This evolutionary stage is associated with particles escaping the PWN and entering the ISM, suggesting this object may be an important source of Galactic PeV e+/e- |
| title | Detection of Diffuse Radio Emission inside the Supernova Remnant G338.3-0.0 associated with the Gamma-ray Source HESS J1640-465 |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2508.18999 |