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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Váldodahkkit:	Yun-Peng Li, Da-Bin Lin, Ning-Yuan Zhang, En-Wei Liang
Materiálatiipa:	Artigo
Giella:	Inglês
Almmustuhtton:	IOP Publishing 2026-01-01
Ráidu:	The Astrophysical Journal
Fáttát:	Gamma-ray bursts Pulsar wind nebulae Neutron stars Jets
Liŋkkat:	https://doi.org/10.3847/1538-4357/ae6f11
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