Finding the missing piece in the Connection between HESSJ1825--178 and G18.0-0.7

Details Finding the missing piece in the Connection between HESSJ1825--178 and G18.0-0.7 Finding the missing piece in the Connection between HESSJ1825--178 and G18.0-0.7

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006xmm..prop..151f&link_type=abstract

XMM-Newton Proposal ID #05039401

Physics

Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, Hess J1825-137, Xmm-Newton Proposal 05039401

Scientific paper

The PWN surrounding the energetic pulsar PSR B1823-13, was found in XMM-Newton observations in 2003. Subsequently the very high-energy (VHE) gamma-ray source HESS J1825-137 was by H.E.S.S. The gamma-ray emission like the X-ray emission extends asymmetrically to the south of the energetic pulsar PSR B1823-13 albeit on a much larger (factor 10) angular scale. The peak of the gamma-ray emission lies in a region never covered by targeted X-ray observations and the existing X-ray data are insufficient to test for a larger extension of the PWN. If the X-ray PWN was in fact larger than previously realised without exhibiting the expected spectral change, or if there was even an additional unrelated X-ray source coincident with the peak of the HESS emission, this whole association

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