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Abt , H · 1983 · arXiv 0183.00201

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astro-ph.HE 1

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A binary origin of ultra-long period radio pulsars

astro-ph.HE · 2025-07-01 · conditional · novelty 6.0

Wind-fed accretion in wide massive binaries can spin neutron stars down past 1000 s, and supernova disruption of the binary then leaves isolated ultra-long period pulsars at a rate of about 10^-6 per year.

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  • A binary origin of ultra-long period radio pulsars astro-ph.HE · 2025-07-01 · conditional · none · ref 4

    Wind-fed accretion in wide massive binaries can spin neutron stars down past 1000 s, and supernova disruption of the binary then leaves isolated ultra-long period pulsars at a rate of about 10^-6 per year.