Magnetic structure of the remnant of Tycho's supernova (SN 1572)

Details Magnetic structure of the remnant of Tycho's supernova (SN 1572) Magnetic structure of the remnant of Tycho's supernova (SN 1572)

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aj....103.1338w&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 103, April 1992, p. 1338-1345.

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Stellar Magnetic Fields, Supernova Remnants, Computational Astrophysics, Magnetic Field Configurations, Radio Emission

Scientific paper

The local magnetic field of Tycho's supernova remnant (3C10) is organized into cell-like regions correlated with regions of relatively high polarized intensity. The size scale of the largest region of locally organized field is about 110 arcsec (1.33 pc), and an apparent size scale of the local field organization of the ambient interstellar medium is about 30 arcsec (0.36 pc). The direction of the mean field in regions of high local field organization within the SNR rim defined by high total intensity is generally radial.

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