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Properties of the Magneto-ionic Medium in the Halo of M51 Revealed by Wide-band Polarimetry

  • Authors: S. A. Mao, E. Zweibel, A. Fletcher, J. Ott, and F. Tabatabaei

Mao et al. 2015 The Astrophysical Journal 800 92.

  • Provider: AAS Journals

Caption: Figure 4.

Polarized emission of source J1330+4703b and the corresponding best fit (solid line) to the uniform external Faraday screen model. We show the fractional Q (filled squares) and U (filled circles) vs. λ2 in the top left plot. The top right plot shows the Q/I-U/I track. The bottom left plot shows the fractional polarization vs. λ2 trend. The bottom right plot shows how polarization angles vary across L band.

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