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A PROPER MOTION FOR THE PULSAR WIND NEBULA G359.23–0.82, THE “MOUSE,” ASSOCIATED WITH THE ENERGETIC RADIO PULSAR J1747–2958
The "Mouse" (PWN G359.23-0.82) is a spectacular bow shock pulsar wind nebula, powered by the radio pulsar J1747-2958. The pulsar and its nebula are presumed to have a high space velocity, but their proper motions have not been directly measured. Here we present 8.5 GHz interferometric observations of the Mouse …