Fig. 8
Radio continuum spectrum for the pulsar wind nebula (PWN) around CXOU J061705.3+222127 in the SNR IC 443. A weighted fit to the data with a single power law function (S ∝ να) yields a spectral index α = −0.04 ± 0.05. The filled circles symbols are from the flux density estimates at 330 and 1420 MHz presented in the current work, while the open symbols are from Olbert et al. (2001).
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