Measuring the magnetic field in SN 1006

Details Measuring the magnetic field in SN 1006 Measuring the magnetic field in SN 1006

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011rmxac..40..201r&link_type=abstract

XIII Latin American Regional IAU Meeting (Eds. W. J. Henney & S. Torres-Peimbert) Revista Mexicana de Astronomía y Astrofísica (

Astronomy and Astrophysics

Astronomy

Ism: Individual (Sn 1006), Ism: Supernova Remnants, Magnetic Fields, Polarization

Scientific paper

We show that the magnetic field in SN 1006 is radial at the bright lobes
but tangential at the SE of the radio shell, where the fractional
polarization is highest. This result suggests that the strongest
particle injection/acceleration occurs in parallel shocks and that the
bright lobes represent polar caps.

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