Morphological Studies of the PWN Candidate HESS J 1809-193

  • N U. K OMIN, Susana Arrigan, +5 authors FOR THE H. E. S. S. C OLLABORATION
  • Published 2008

Abstract

The source HESS J1809−193 was discovered in 2006 in data of the Galactic Plane survey, followed by several re-observations. It shows a hard gamma-ray spectrum and the emission is clearly extended. Its vicinity to PSR J1809-1917, a high spin-down luminosity pulsar powerful enough to drive the observed gamma-ray emission, makes it a plausible candidate for a… (More)

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