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DETECTION OF THE ENERGETIC PULSAR PSR B1509–58 AND ITS PULSAR WIND NEBULA IN MSH 15–52 USING THE<i>FERMI</i>-LARGE AREA TELESCOPE
We report the detection of high-energy γ-ray emission from the young and energetic pulsar PSR B1509 − 58 and its pulsar wind nebula (PWN) in the composite supernova remnant G320.4 − 1.2 (aka MSH 15 − 52). Using 1 yr of survey data with the Fermi-Large Area Telescope (LAT), we …