Modelling of the surface emission of the low magnetic field magnetar SGR 0418+5729
We perform a detailed modelling of the post-outburst surface emission of the low magnetic field magnetar SGR 0418+5729. The dipolar magnetic field of this source, B = 6 x 10(12) G estimated from its spin-down rate, is in the observed range of magnetic fields for normal pulsars. The source is further...
| Autores principales: | , , , , |
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| Formato: | Artículo (Article) |
| Idioma: | Inglés (English) |
| Publicado: |
2025
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| Materias: | |
| Acceso en línea: | https://repositorio.uc.cl/handle/11534/101527 |