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- W1566963295 abstract "S>Synthesis observations made with the Westerbork telescope were used to produce maps of the supernova remnants 3 C 10 and 3 C 461. The Stokes parameters I, Q, and U were determined with a resolution of about 25''. The total intensity map of 3 C 10 showed significant emission from the remnant's center, and the results can be approximately reproduced by a spherical shell of synchrotron emitting material. The best shell model, whose thickness is one-fourth of its outer radius, also requires that the magnetic fields have an ordered component predominantly in the radial direction. Such a configuration, which has been previously suggested for 3 C 461, is in accord with high frequency polarization measurements. The degree of linear polarization from 3 C 461 was generally under 1%. The polarization of Tycho's remnant is dominated by a cellular structure wherein the position angle remains constant within regions of about 1' diameter, while large changes can occur between adjacent regions. The degree of polarization within cells, running as high as 14%, was virtually the same as that obtained at higher frequencies. The interpretation most consistent with the data is that differential Faraday rotation occurs in a thin screen surrounding the remnant,more » and this is identified with magneto-ionic material swept up from the interstellar medium. Thus the shell of relativistic particles is surrounded by a thin, relatively dense screen of hot gas which produces the differential rotation, the weak optical emission, and, presumably, the soff x-ray emission. (auth)« less" @default.
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- W1566963295 date "1973-06-01" @default.
- W1566963295 modified "2023-09-28" @default.
- W1566963295 title "High resolution 21 cm continuum study of the supernova remnants 3C 10 (Tycho's Supernova Remnant) and 3C 461 (Cas A)" @default.
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