Magnetic Fields in Supernova Remnants

Details Magnetic Fields in Supernova Remnants Magnetic Fields in Supernova Remnants

Feb 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004mim..proc..141f&link_type=abstract

The Magnetized Interstellar Medium, Proceedings of the conference, held in Antalya, Turkey, September 8 - 12, 2003, Eds: B. Uyan

Physics

8

Scientific paper

Observations of the polarized radio emission from supernova remnants are reviewed. Some characteristics of the deduced intrinsic magnetic fields are listed and used to determine the role of the magnetic field for the dynamics of these objects. The relation between the magnetic fields of SNRs and the Galactic magnetic field local to the SNRs is considered. Typical properties of the magnetic field of the various SNR classes are discussed. Recent results of OH Zeeman splitting observations indicate milli-Gauss magnetic fields in filamentary structures.

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