Multiwavelength Emission for a Postmerger Magnetar: The Magnetar-driven Poynting Jet and Its Associated Pulsar Wind Nebula
A newly born, rapidly rotating magnetar may form in a binary neutron star merger and drive a Poynting flux-dominated relativistic jet. As the jet propagates outward, a forward shock (FS) and a reverse shock (RS) are formed, inflating a pulsar wind nebula (PWN) between them. We present a systematic s...
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| Principais autores: | , , , |
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| Format: | Artigo |
| Sprog: | Inglês |
| Udgivet: |
IOP Publishing
2026-01-01
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| Serier: | The Astrophysical Journal |
| Fag: | |
| Online adgang: | https://doi.org/10.3847/1538-4357/ae6f11 |
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