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

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142 Data reduction and imaging of lobed radio galaxies 0 2 4 6 8 10 12 54 30 00 53 30 DECLINATION (J2000) 00 52 30 00 51 30 12 25 09 08 07 06 05 04 03 02 01 RIGHT ASCENSION (J2000) p = 1 12 25 09 08 07 06 05 04 03 02 01 RIGHT ASCENSION (J2000) Figure 13: Images of M 84 at 1.65 arcsec resolution. Left: Total intensity at 4.9 GHz in mJy (beam area) −1 . Right: Apparent B a vectors with lengths proportional to p 4.9 derived from the 4-frequency RM fits at 4.5 arcsec, superimposed on a false-colour display of the total intensity gradient at 4.9 GHz. 90 ◦ in projection. Lower-resolution observations were previously shown by Laing & Bridle (1987) so are not repeated here. The right panel of Fig. 13 shows the apparent magnetic field structure. In the N lobe, the magnetic field is predominantly perpendicular to the presumed path of the jet along its mid-line. The magnetic field in the S lobe is broadly circumferential and a sudden increase in the degree of polarization at the edge of the lobe is apparent. 142
Bibliography Ackermann, M., Ajello, M., Allafort, A., Baldini, L., et al., 2010, ApJ, 717, 127 Allen, S. W., Taylor, G. B., Nulsen, P. E. J., Johnstone, R. M., et al. 2001, MNRAS, 324, 842 Andernach, H., Feretti, L., Giovannini, G. et al. 1992, A&A, 93, 331 Antonucci, R., 1993, ARA&A, 31, 473 Baars J.W.M., Genzel R., Pauliny-Toth I.I.K., Witzel, A., 1977, A&A, 61, 99 Balbus, S. A. 2000, ApJ, 534, 420 Barthel, P., 1989, SciAm, 260, 20 Bagchi, J., Durret, F., Lima Neto, G.B., Paul, S. 2006, Science, 314, 791 Baum, Stefi Alison, Heckman, Timothy M., Bridle, Alan, van Breugel, Wil J. M., Miley, George K, 1988, ApJS, 68, 643 Beck R., 1996, ASPC, 97, 475 Beck R. & Krause M., 2005, AN, 326, 414 Bicknell, G.V., 1994, ApJ, 422, 542 Bicknell, G.V., Cameron, R.A. & Gingold, R.A., 1990, ApJ, 357, 373 Biermann, P., Kronberg, P. P. & Madore, B. F., 1982, ApJ, 256, 37 Binney, J., Tabor, G., 1995, MNRAS, 276, 663 Biretta J.A., Zhou F. & Owen F.N., 1995, ApJ, 447, 582 Biretta, J.A., Sparks, W.B. & Macchetto, F., 1999, ApJ, 520, 621 Birkinshaw, M., Laing, R. A. & Peacock, J. A. 1981, MNRAS, 197, 253 143
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Alma Mater Studiorum Università de
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To Hypatia from Alexandria in Egypt
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Contents Abstract i 1 Physics of ra
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4.6.3 The outer scale of the magnet
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Abstract The existence of diffuse m
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2. Two-dimensional Monte Carlo simu
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Chapter 1 Physics of radio galaxies
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1.2. Non-thermal emission mechanism
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1.2. Non-thermal emission mechanism
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1.3. Radio galaxies 7 FR II sources
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1.3. Radio galaxies 9 (a) (b) Figur
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1.3. Radio galaxies 11 pressure, th
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Chapter 2 The X-ray environment of
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2.2. The thermal component 15 Figur
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2.3. Radio source - environment int
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2.3. Radio source - environment int
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Chapter 3 Magnetic fields in the ho
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3.1. Introduction 23 Figure 3.1: Ex
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3.1. Introduction 25 to the relativ
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3.2. Faraday Rotation 27 The RM can
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3.2. Faraday Rotation 29 Figure 3.4
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3.3. Depolarization 31 3.3 Depolari
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3.5. The magnetic field profile 33
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3.6. Tangled magnetic field 35 rad
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3.7. The magnetic field power spect
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Chapter 4 Structure of the magneto-
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4.1. The radio source 3C 449: gener
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4.3. The Faraday rotation in 3C 449
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4.3. The Faraday rotation in 3C 449
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4.4. Depolarization 51 Figure 4.4:
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4.4. Depolarization 53 1.25 arcsec
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4.5. Two dimensional analysis 55 sm
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4.5. Two dimensional analysis 57 Fi
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4.6. Three-dimensional analysis 59
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4.7. Summary and comparison with ot
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Chapter 5 Ordered magnetic fields a
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5.1. The Sample 75 35 49 00 ROSAT P
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5.1. The Sample 77 5.1.1 0206+35 02
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5.2. Analysis of RM and depolarizat
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5.3. Rotation measure images 81 IMA
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5.3. Rotation measure images 83 cor
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5.4. Depolarization 85 Therefore, a
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5.5. Rotation measure structure fun
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5.6. Rotation-measure bands from co
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Page 115 and 116: 5.8. Discussion 99 5.8 Discussion 5
Page 117 and 118: 5.8. Discussion 101 line−of−sig
Page 119 and 120: 5.8. Discussion 103 flat slopes. I
Page 121 and 122: 5.9. Conclusions and outstanding qu
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Page 125 and 126: Chapter 6 Faraday rotation in two e
Page 127 and 128: 6.2. Two-dimensional analysis: rota
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Page 137 and 138: 6.4. Preliminary conclusions 121 Ta
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Page 141 and 142: Summary and conclusions The goal of
Page 143 and 144: 6.5. Summary 127 responsible for th
Page 145 and 146: 6.6. General conclusions 129 radio
Page 147 and 148: 6.7. Future prospects 131 and is th
Page 149: Appendix 133
Page 152 and 153: 136 Data reduction and imaging of l
Page 160 and 161: 144 BIBLIOGRAPHY Bîrzan, L., Raffe
Page 162 and 163: 146 BIBLIOGRAPHY Ensslin, T.A. & Go
Page 164 and 165: 148 BIBLIOGRAPHY Jeltema, T.E. & Pr
Page 166 and 167: 150 BIBLIOGRAPHY Owen, F.N., 1989,
Page 168 and 169: 152 BIBLIOGRAPHY 152
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