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      PSR J2030+4415's Remarkable Bow Shock, PWN and Filament

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          Abstract

          We report on new X-ray and optical observations of PSR J2030+4415, a Gamma-ray Pulsar with an H\(\alpha\) bow shock. These data reveal the velocity structure of the bow shock apex and resolve unusual X-ray structure in its interior. In addition the system displays a very long, thin filament, extending at least \(5^\prime\) at \(\sim 130^\circ\) to the pulsar motion vector. Careful astrometry, compared with a short archival exposure, detects the pulsar proper motion at 85 mas yr\(^{-1}\). With the H\(\alpha\) velocity structure this allows us to estimate the distance as \(0.75\) kpc.

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          Author and article information

          Journal
          27 May 2020
          Article
          2005.13572
          7268f972-c531-4a6d-b2f8-24a966bbaf04

          http://creativecommons.org/licenses/by/4.0/

          History
          Custom metadata
          6 pages, 4 figures. Accepted for publication in ApJL
          astro-ph.HE

          High energy astrophysical phenomena
          High energy astrophysical phenomena

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