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Properties of the Magneto-ionic Medium in the Halo of M51 Revealed by Wide-band Polarimetry
Mao et al.
2015 The Astrophysical Journal 800
Caption: Figure 5.
Polarized emission of source J1329+4717 and the corresponding best fit (solid line) to the inhomogeneous external Faraday screen model. This figure has the same layout as in Figure 4.
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