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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6.2. Two-<strong>di</strong>mensional analysis: rotation measure and depolarization 117<br />
IMAGE: M87.RMRAL_BLANK.FITS<br />
DECLINATION (J2000)<br />
12 23 45<br />
12 23 30<br />
12 23 15<br />
12 23 00<br />
;2000 0 2000 4000 6000<br />
RAD/M/M<br />
1 kpc<br />
12 22 45<br />
12 30 52<br />
12 30 51<br />
12 30 50 12 30 49 12 30 48<br />
RIGHT ASCENSION (J2000)<br />
12 30 47<br />
Figure 6.7: Rotation measure of M 87 computed from fits to the position angle –λ 2 rotation at<br />
eight frequencies as described in the text. The angular resolution is 0.4 arcsec FWHM.<br />
The new map, shown in Fig. 6.7, has an average fitting errorσ RMfit = 15 rad m −2 . The RM<br />
<strong>di</strong>stribution has a mean of roughly 650 rad m −2 withσ RM ≈900 rad m −2 .<br />
The main features of the RM image are as follows.<br />
• The RM values are large and almost always positive, requiring a magnetic field pointing<br />
towards us across most of the source. They range from≈−2000 up to≈6000 rad m −2 . This<br />
compares with the much larger range of−1000-8000 rad m −2 found by Owen, Eilek & Keel<br />
(1990). The most extreme positive values found by are Owen, Eilek & Keel (1990) not<br />
consistent with the X-band position angles.<br />
• The highest RM values (≈3500-6000 rad m −2 ) are seen only in a restricted patch in the E<br />
lobe.<br />
• The jet appears as a uniform RM structure characterized by low values (≈100 rad m −2 ), as<br />
already pointed out by Owen, Eilek & Keel (1990).<br />
• The RM <strong>di</strong>stribution is asymmetrical: positive and smoothly varying in the W lobe, patchier<br />
and associate with field reversals in the E lobe.<br />
As in 0755+37, the low RM seen across the jet is surprising. Similar explanations may hold<br />
for the two sources.<br />
117