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Alma Mater Studiorum Universit`a degli Studi di Bologna ... - Inaf

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118 6. Faraday rotation in two extreme environments<br />

0 20000 40000 60000<br />

12 24 00<br />

12 23 40<br />

DECLINATION (J2000)<br />

12 23 20<br />

12 23 00<br />

12 22 40<br />

12 30 51<br />

12 30 50<br />

12 30 49<br />

12 30 48<br />

12 30 47<br />

RIGHT ASCENSION (J2000)<br />

Figure 6.8: Left: Image of Burn law k for M 87 computed from weighted least-squares fits to the<br />

relation p(λ)= p(0)exp(−kλ 4 ) at the eight frequencies listed in Table 6.3. Right: Profiles of Burn<br />

law k along the jet <strong>di</strong>rection, plotted against <strong>di</strong>stance from the nucleus. The angular resolution is<br />

0.4 arcsec FWHM.<br />

The Burn law k map for M 87 is shown in Fig. 6.8. At 0.4 arcsec resolution the overall k<br />

<strong>di</strong>stribution has a mean of 9820 rad 2 m −4 , correspon<strong>di</strong>ng to a depolarization DP 6cm<br />

3cm<br />

= 0.85. The<br />

mean observed k values for the two lobes are listed in Table 6.4. The highest depolarization occurs<br />

in patchy structures in the E (rece<strong>di</strong>ng) lobe, consistent with the Laing-Garrington effect (Laing<br />

1988; Garrington et al. 1988). These structures appear filamentary and are likely to be caused by<br />

steep (and therefore unresolved) RM gra<strong>di</strong>ents. Indeed, they are in the same areas as the highest<br />

absolute values of RM and∇RM (Fig. 6.7).<br />

In ad<strong>di</strong>tion to low and constant RM, the jet also shows uniformly low k.<br />

The profile of<br />

〈k〉 across the source (Fig. 6.8, right) is qualitatively similar to that observed in 0755+37, but<br />

more extreme: it increases monotonically from W to E across the core, peaks in the E lobe<br />

and then decreases at larger <strong>di</strong>stances. Except in the region of the jet, no detailed correlation<br />

of depolarization with source morphology is apparent. Together with the absence of significant<br />

deviations fromλ 2 rotation, this again requires a Faraday rotating me<strong>di</strong>um mostly external to the<br />

source.<br />

6.3 Two-<strong>di</strong>mensional analysis: structure functions<br />

I used the RM structure function (Eq. 3.13) to quantify the two-<strong>di</strong>mensional fluctuations of Faraday<br />

rotation measure on scales larger than the observing beamwidth for 0755+37 and M 87.<br />

118

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