Radio Emission across the Entire Rotation Phases of Pulsars
Supersensitive observations of bright pulsars by the Five-hundred-meter Aperture Spherical Telescope have revealed weak radio emission continuously emerges in the rotation phases between the “main” pulse and “interpulse” of a rotating neutron star. We develop a model for the polarized radio emission...
Guardat en:
| Autors principals: | , |
|---|---|
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
IOP Publishing
2025-01-01
|
| Col·lecció: | The Astrophysical Journal |
| Matèries: | |
| Accés en línia: | https://doi.org/10.3847/1538-4357/adc9a6 |
| Etiquetes: |
Sense etiquetes, Sigues el primer a etiquetar aquest registre!
|