Measurement of Spectral Breaks in Pulsar Wind Nebulae with Millimeter‐Wave Interferometry
Measurement of Spectral Breaks in Pulsar Wind Nebulae with Millimeter‐Wave Interferometry
We have observed pulsar wind nebulae (PWNe) in the three supernova remnants G11.2-0.3, G16.7+0.1, and G29.7-0.3 at 89 GHz with the Berkeley-Illinois-Maryland Association array, measuring total flux densities of two of them for comparison with archival data at other frequencies. In G16.7+0.1, we find a break in the spectrum of …