PSR J0002+6216 explained

PSR J0002+6216, also dubbed the Cannonball Pulsar, is a pulsar discovered by the Einstein@Home project in 2017.[1] It is one of the fastest moving pulsars known, and has moved 53ly away from the location of its formation supernova, where the remaining supernova nebula, CTB 1 (Abell 85[2]), is. Due to its speed in traversing the interstellar medium, at 1127km/s, it is leaving a 13ly long wake tail and is traveling fast enough to leave the Milky Way galaxy. The pulsar is currently 6500ly away in the Cassiopeia constellation. The star rotates at a rate of 8.7 times a second.[3] [4] There is bow-shock pulsar wind nebula (PWN) associated with PSR J0002+6216. [5]

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Notes and References

  1. Schinzel . F. K. . Kerr . M. . Rau . U. . Bhatnagar . S. . Frail . D. A. . The Tail of PSR J0002+6216 and the Supernova Remnant CTB 1 . The Astrophysical Journal . American Astronomical Society . 876 . 1 . 2019-05-03 . 2041-8213 . 10.3847/2041-8213/ab18f7 . L17. free . 1904.07993 .
  2. Web site: Abell 85 . AstroSurf .
  3. News: Astronomers Find Pulsar Hurtling Through Space . 22 March 2019 . Sci-News.com .
  4. Web site: Astronomers Find "Cannonball Pulsar" Speeding Through Space . Dave Finley . National Radio Astronomy Observatory . 19 March 2019 .
  5. Kumar . P. . Schinzel . F. K. . Taylor . G. B. . Kerr . M. . Castro . D. . Rau . U. . Bhatnagar . S. . Resolving the Bow Shock and Tail of the Cannonball Pulsar PSR J0002+6216 . The Astrophysical Journal . American Astronomical Society . 945 . 2 . 2023-03-01 . 0004-637X . 10.3847/1538-4357/acba93 . 129. free . 2302.04927 .