Radio polarization in the supernova remnant Puppis A (G 260.4 - 3.4)

Details Radio polarization in the supernova remnant Puppis A (G 260.4 - 3.4) Radio polarization in the supernova remnant Puppis A (G 260.4 - 3.4)

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993mnras.261..366m&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 261, no. 2, p. 366-370.

Astronomy and Astrophysics

Astronomy

4

Polarization (Waves), Radio Astronomy, Supernova Remnants, Faraday Effect, Interstellar Magnetic Fields

Scientific paper

We present a radio polarization study of the young supernova remnant
Puppis A (G 260.4 - 3.4). A radial magnetic field, consistent with its
young age, and moderately low negative values for the rotation measure
are deduced. There is little depolarization over this SNR.

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