Berlin 2005 – wissenschaftliches Programm

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T: Teilchenphysik

T 202: Kosmische Strahlung II

T 202.5: Vortrag

Freitag, 4. März 2005, 15:00–15:15, TU H106

Observation of MSH 15-5-02 at the TeV range with the H.E.S.S. detector — •Bruno Khelifi — MPIK Heidelberg, Postfach 103980, 69029 Heidelberg

The system MSH 15-5-02 is a composite object made by the supernova remnant G320.4-1.2 and by the energetic pulsar PSR B1509-58. A pulsar wind nebula around this pulsar has been detected in radio and X-ray wavelengths. In March/June 2004, MSH 15-5-02 was observed at TeV energies with the H.E.S.S. Cherenkov telescope system. The results is interpreted in the framework of a pulsar wind nebula emission.