Radio polarization of the VELA X supernova remnant

Details Radio polarization of the VELA X supernova remnant Radio polarization of the VELA X supernova remnant

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....81..293m&link_type=abstract

Astronomy and Astrophysics, vol. 81, no. 3, Jan. 1980, p. 293-301.

Astronomy and Astrophysics

Astronomy

31

Polarized Electromagnetic Radiation, Radio Sources (Astronomy), Supernova Remnants, Depolarization, Faraday Effect, Mathematical Models, Stellar Magnetic Fields

Scientific paper

Maps are presented of the 2.7 and 5 GHz total intensity and the polarization distributions over the large, close, supernova remnant Vela X. Distributions of spectral index, Faraday rotation measure and depolarization ratio are drawn from these data and supplementary observations at 1.6 GHz. The rotation measures and depolarization are generally low; it is suggested that Faraday rotation and most of the depolarization occurs in the outer regions of Vela X.

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