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- W3099028908 abstract "We have carried out Very Large Array imaging and a Fermi timing analysis of the 115 ms γ-ray and radio pulsar PSR J0002+6216. We found that the pulsar lies at the apex of a narrowly collimated cometary-like 7' tail of nonthermal radio emission, which we identify as a bow-shock pulsar wind nebula. The tail of the nebula points back toward the geometric center of the supernova remnant CTB 1 (G116.9+0.2) 28' away, at a position angle θμ = 113°. We measure a proper motion with 2.9σ significance from a Fermi timing analysis giving μ = 115 ± 33 mas yr−1 and θμ = 121° ± 13°, corresponding to a large transverse pulsar velocity of 1100 km s−1 at a distance of 2 kpc. This proper motion is of the right magnitude and direction to support the claim that PSR J0002+6216 was born from the same supernova that produced CTB 1. We explore the implications for pulsar birth periods, asymmetric supernova explosions, and mechanisms for pulsar natal kick velocities." @default.
- W3099028908 created "2020-11-23" @default.
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- W3099028908 date "2019-05-03" @default.
- W3099028908 modified "2023-09-23" @default.
- W3099028908 title "The Tail of PSR J0002+6216 and the Supernova Remnant CTB 1" @default.
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- W3099028908 doi "https://doi.org/10.3847/2041-8213/ab18f7" @default.
- W3099028908 hasPublicationYear "2019" @default.
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