Alma Mater Studiorum Universit`a degli Studi di Bologna ... - Inaf
Alma Mater Studiorum Universit`a degli Studi di Bologna ... - Inaf
Alma Mater Studiorum Universit`a degli Studi di Bologna ... - Inaf
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Chapter 6<br />
Faraday rotation in two extreme<br />
environments ‡<br />
In this Chapter I will present polarization analyses of two ra<strong>di</strong>o galaxies embedded in very<br />
<strong>di</strong>fferent environments. The sources are: B2 0755+37, located in a very sparse group, and<br />
M 87, located at the centre of the cool core Virgo cluster. I will described the results of two<strong>di</strong>mensional<br />
analyses of the RM and depolarization <strong>di</strong>stributions. In both sources, the geometry<br />
of the surroun<strong>di</strong>ng X-ray emitting gas appears to be complex than for the sources stu<strong>di</strong>ed in<br />
Chapters 4 and 5, so a three-<strong>di</strong>mensional analysis will be deferred to a later study.<br />
6.1 The sources<br />
The general parameters of the sources are listed in Table 6.1, while Table 6.2 shows the X-ray<br />
parameters taken from the literature and the equipartition parameters derived from ra<strong>di</strong>o data in<br />
this work. I refer to parts of the sources by the abbreviations N, S, E, W (for North, South, East,<br />
West).<br />
6.1.1 B2 0755+37<br />
B2 0755+37 (hereafter 0755+37) is an extended FR I ra<strong>di</strong>o source whose optical counterpart,<br />
NGC 2484, is a D-galaxy, classified as central member of a nearby and very poor group of galaxies<br />
(Mulchaey et al. 2003). The source is one of the most isolated ra<strong>di</strong>o galaxies in the B2 catalogue.<br />
Here I briefly summarize the ra<strong>di</strong>o properties of 0755+37, which are described in detail in the<br />
Appen<strong>di</strong>x of this thesis along with a description of the VLA observations. At a resolution of<br />
‡ Guidetti et al. in prep<br />
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