A closer look at HESS J1837-069 following the pulsar discovery

Details A closer look at HESS J1837-069 following the pulsar discovery A closer look at HESS J1837-069 following the pulsar discovery

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1085..320m&link_type=abstract

HIGH ENERGY GAMMA-RAY ASTRONOMY: Proceedings of the 4th International Meeting on High Energy Gamma-Ray Astronomy. AIP Conferenc

Astronomy and Astrophysics

Astronomy

Astronomical And Space-Research Instrumentation, Pulsars, Gamma-Ray Sources, Gamma-Ray Bursts

Scientific paper

The gamma-ray source HESS J1837-069 was discovered during the first scan of the galactic plane, and was classified as an unidentified source, possibly associated with AX J1838.0-0655. Recently, an energetic 23 kyr pulsar was discovered in coincidence with the ASCA source. We present a preliminary analysis of a larger HESS data set which reveals finer morphology and spectral details. We discuss the pulsar wind nebula (PWN) interpretation of the gamma-ray source in view of the characteristics of other very high energy (VHE) emitting pulsar wind nebula.

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