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...
Gorde:
| Egile Nagusiak: | , |
|---|---|
| Formatua: | Artigo |
| Hizkuntza: | Inglês |
| Argitaratua: |
IOP Publishing
2025-01-01
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| Saila: | The Astrophysical Journal |
| Gaiak: | |
| Sarrera elektronikoa: | https://doi.org/10.3847/1538-4357/adc9a6 |
| Etiketak: |
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