Glitch time series and size distributions in eight prolific pulsars
Context. Glitches are rare spin-up events that punctuate the smooth slow-down of the rotation of pulsars. For the Vela pulsar and PSR J0537-6910, their large glitch sizes and the times between consecutive events have clear preferred scales (Gaussian distributions), contrary to the handful of other p...
| 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/11534/100752 |