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

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152 BIBLIOGRAPHY 152
Acknowledgments Probably the most important result is that during this PhD I have grown not only as scientist but as person. For this, I owe many people a debt of gratitude for all my life. I am privileged for having Robert Laing as supervisor, this thesis would not have been possible without his help and patience. I have learned many valuable things from him, and I also wish to express gratitude for believing in me. One simply could not wish for a better supervisor. I thank Paola Parma and Loretta Gregorini for their help and support. I would like to acknowledge ESO (Garching) for the award of a ESO Studentship that allowed me to breath a wide spirit of research and to grow. I wish to thank Matteo Murgia, Federica Govoni and the staff of the Astronomical Observatory of Cagliari for their hospitality and support during the development of the work on 3C 449. The work on this radio galaxy is part of the “Cybersar” Project, which is managed by the COSMOLAB Regional Consortium with the financial support of the Italian Ministry of University and Research (MUR), in the context of the “Piano Operativo Nazionale Ricerca Scientifica, Sviluppo Tecnologico, Alta Formazione (PON 2000-2006)”. I wish to thank Luigina Feretti for providing the excellent VLA dataset of 3C 449 and Greg Taylor for the use of his rotation measure code. I also thank M. Swain for providing the VLA dataset for 3C 353, J. Eilek for a FITS image of 3C 465 and J. Croston, A. Finoguenov and J. Goodger for the FITS images of 3C 270, M 84 and 3C 353, respectively. I am grateful to M. Bondi, G. Brunetti, A. Shukurov and J. Stöckl for many valuable comments. I also acknowledge the use of HEALPIX package (http://healpix.jpl.nasa.gov) and the provision of the models of Dineen & Coles (2005) inHEALPIX format. The last but certainly not least words are for all of You which “see all my light and love my dark”. “And thus I stand”. 153
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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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5.7. Rotation-measure bands from a
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5.7. Rotation-measure bands from a
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5.8. Discussion 99 5.8 Discussion 5
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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
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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,
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