Multi-frequency radio-continuum study of the LMC SNR N206 (Goat's Eye) and its "zig-zag" PWN
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2025
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| author | Ghavam, M. Smeaton, Z. J. Filipovic, M. D. Alsaberi, R. Z. E. Bordiu, C. Cotton, W. D. Crawford, E. J. Hopkins, A. M. Kothes, R. Lazarevic, S. Leahy, D. Rajabpour, N. Ranasinghe, S. Rowell, G. P. Sano, H. Sasaki, M. Shobhana, D. Tsuge, K. Urosevic, D. Tothill, N. F. H. |
| author_facet | Ghavam, M. Smeaton, Z. J. Filipovic, M. D. Alsaberi, R. Z. E. Bordiu, C. Cotton, W. D. Crawford, E. J. Hopkins, A. M. Kothes, R. Lazarevic, S. Leahy, D. Rajabpour, N. Ranasinghe, S. Rowell, G. P. Sano, H. Sasaki, M. Shobhana, D. Tsuge, K. Urosevic, D. Tothill, N. F. H. |
| contents | We present new radio-continuum observations of the Large Magellanic Cloud (LMC) supernova remnant (SNR) N206, which we give the name "Goat's Eye". Goat's Eye contains an interior radio structure that is likely a pulsar wind nebula (PWN), which we analyse in further detail. We use new radio observations from the Australia Telescope Compact Array (ATCA) telescope, as well as several archival radio observations, to calculate spectral indices, and find a steep spectral index for the whole SNR ($α= -0.60\pm0.02$), and a flatter spectral index for the PWN ($α= -0.16\pm0.03$). We also measure the polarisation and magnetic field properties of the PWN. Previously reported as a linear structure, the new observations show an unusual "zig-zag"-like structure, visible in radio-continuum total intensity, linear polarisation, and magnetic field orientations. The origin of this zig-zag structure is unclear, but we propose some origin scenarios that will require further observations to differentiate between. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2512_01221 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Multi-frequency radio-continuum study of the LMC SNR N206 (Goat's Eye) and its "zig-zag" PWN Ghavam, M. Smeaton, Z. J. Filipovic, M. D. Alsaberi, R. Z. E. Bordiu, C. Cotton, W. D. Crawford, E. J. Hopkins, A. M. Kothes, R. Lazarevic, S. Leahy, D. Rajabpour, N. Ranasinghe, S. Rowell, G. P. Sano, H. Sasaki, M. Shobhana, D. Tsuge, K. Urosevic, D. Tothill, N. F. H. High Energy Astrophysical Phenomena We present new radio-continuum observations of the Large Magellanic Cloud (LMC) supernova remnant (SNR) N206, which we give the name "Goat's Eye". Goat's Eye contains an interior radio structure that is likely a pulsar wind nebula (PWN), which we analyse in further detail. We use new radio observations from the Australia Telescope Compact Array (ATCA) telescope, as well as several archival radio observations, to calculate spectral indices, and find a steep spectral index for the whole SNR ($α= -0.60\pm0.02$), and a flatter spectral index for the PWN ($α= -0.16\pm0.03$). We also measure the polarisation and magnetic field properties of the PWN. Previously reported as a linear structure, the new observations show an unusual "zig-zag"-like structure, visible in radio-continuum total intensity, linear polarisation, and magnetic field orientations. The origin of this zig-zag structure is unclear, but we propose some origin scenarios that will require further observations to differentiate between. |
| title | Multi-frequency radio-continuum study of the LMC SNR N206 (Goat's Eye) and its "zig-zag" PWN |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2512.01221 |