THE RADIO COUNTERPART OF THE X-RAY PULSAR WIND NEBULA IN THE SNR G0.9+0.1

摘要

We report on new radio observations of the central nebula in the SNR G0.9+0.1 at 4.8GHz and 8.6GHz. These data unveil a highly clumpy structure of the radio nebula. Most of the radio features are uncorrelated with the X-ray emission. Not any point-like radio source is detected at the position of CXOU J174722.8-280915, the proposed neutron star. On the contrary, the X-ray source seems to lie within a small minimum in the radio emission.