The Radio Properties and Magnetic Field Configuration in Pulsar Wind Nebula G54.1+0.3

Details The Radio Properties and Magnetic Field Configuration in Pulsar Wind Nebula G54.1+0.3 The Radio Properties and Magnetic Field Configuration in Pulsar Wind Nebula G54.1+0.3

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...20915914l&link_type=abstract

2007 AAS/AAPT Joint Meeting, American Astronomical Society Meeting 209, #159.14; Bulletin of the American Astronomical Society,

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We present multifrqeuency radio observations made with the Very Large Array of the pulsar wind nebula known as SNR G54.1+0.3. Radio spectral index and morphological results provide insight into the energetics of this Crab-like PWN. However, unlike the Crab, the radio and X-ray extents are very similar. We present a discussion of the comparisons between the high-resolution Chandra X-ray image and the radio images. We also present high-resolution ( 5") radio polarimetric results which illustrate the intrinsic magnetic field structure of the PWN. Few such studies have been done for PWNe. The magnetic field in G54.1+0.3 appears to be highly ordered and well organized.

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