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Title:
Magnetic structure of the remnant of Tycho's supernova (SN 1572)
Authors:
Wood, Craig A.; Mufson, Stuart L.; Dickel, John R.
Affiliation:
AA(Indiana University, Bloomington), AB(Indiana University, Bloomington), AC(Illinois, University, Urbana)
Publication:
Astronomical Journal (ISSN 0004-6256), vol. 103, April 1992, p. 1338-1345. (AJ Homepage)
Publication Date:
04/1992
Category:
Astrophysics
Origin:
STI
NASA/STI Keywords:
STELLAR MAGNETIC FIELDS, SUPERNOVA REMNANTS, COMPUTATIONAL ASTROPHYSICS, MAGNETIC FIELD CONFIGURATIONS, RADIO EMISSION
DOI:
10.1086/116147
Bibliographic Code:
1992AJ....103.1338W

Abstract

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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