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Investigations of Faraday Rotation Maps of Extended Radio Sources ...

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30 CHAPTER 2. IS THE RM SOURCE-INTRINSIC OR NOT?<br />

Figure 2.1: This plot is adapted from Rudnick & Blundell (2003) and shows polarisation<br />

structures <strong>of</strong> the source PKS 1246-410. The source is ≈ 30 ” long. Left column:<br />

Original data from Taylor et al. (2002) after applying a median weight filter. Top:<br />

polarised intensity at 8 GHz, peak flux density 4 mJy/beam (red); middle rotation<br />

measures ≈ − 1300 (blue) to 1300 (red) rad/m 2 ; bottom: intrinsic polarisation angle<br />

ϕ 0 − 90 ◦ (blue) to 90 ◦ (red). Right Column: three different simulations <strong>of</strong> rotation<br />

measures having the same colour coding as the actual rotation measures have. Note the<br />

different patchiness <strong>of</strong> the simulated rotation measure images compared to the original<br />

data although they share the same RM power spectrum.<br />

Taylor et al. (2002), which is shown in the middle left panel <strong>of</strong> Fig. 2.1 after applying<br />

a smoothing algorithm. If the RM is generated in a thin dense mixing layer enclosing<br />

the radio source, co-spatial structures in the ϕ 0 and RM distributions are expected. On<br />

the other hand, if the <strong>Faraday</strong> rotation is generated in an external intra-cluster medium<br />

than there should be no correlation observed between RM and ϕ 0 .<br />

Rudnick & Blundell (2003) search for co-spatial structures in the distribution <strong>of</strong><br />

RM and ϕ 0 . For that, they derive RM-ϕ 0 scatter plots in which they compare these<br />

two quantities at each point <strong>of</strong> the image. For the source PKS 1246-410, this scatter<br />

plot is shown in the upper middle panel <strong>of</strong> Fig. 2.2. Rudnick & Blundell argue that<br />

local co-alignment <strong>of</strong> ϕ 0 and RM should lead to strongly clustered point distributions<br />

in such a scatter plot. Since also statistically independent RM and ϕ 0 distributions<br />

may produce such clustering Rudnick & Blundell generate synthetic RM maps having<br />

the same power spectrum as the observed one, but random phases. They repeat their<br />

analysis with these simulated images and find that the scatter plots for the simulated<br />

maps show less clustering. They conclude that the scenario <strong>of</strong> a mixing layer is the<br />

most likely one.

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