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88 Chapter 2. Multiwavelength approach to LS 5039
Bibliography Blandford, R. D., & Königl, A. 1979, ApJ, 232, 34 Blandford, R. D., & Payne, D. G. 1982, MNRAS, 199, 883 Casares, J., Ribó, M., Paredes, J. M., & Martí, J. 2002, in preparation Clark, J. S., Reig, P., Goodwin, S. P., et al. 2001, A&A, 376, 476 Condon, J. J., Cotton, W. D., Greisen, E. W., et al. 1998, AJ, 115, 1693 Deutschman, W. A., Davis, R. J., & Schild, R. E. 1976, ApJS, 30, 97 Distefano, C., Guetta, D., Waxman, E., & Levinson, A. 2002, ApJ, 575, 378 Drilling, J. S. 1975, AJ, 80, 128 Drilling, J. S. 1991, ApJS, 76, 1033 Fender, R. P., & Hendry, M. A. 2000, MNRAS, 317, 1 Fender, R. P., Roche, P., Pooley, G. G., et al. 1997, in Proc. of the 2nd INTEGRAL Workshop ‘The Transparent Universe’, ESA SP-382, 303 Gray, D. F. 1976, The Observations and Analysis of Stellar Photospheres, Wiley- Interscience, New York Hartman, R. C., Bertsch, D. L., Bloom, S. D., et al. 1999, ApJS, 123, 79 Helfand, D. J., Zoonematkermani, S., Becker, R. H., et al. 1980, ApJ, 80, 211 Hjellming, R. M., & Han, X. 1995, Radio properties of X-ray binaries, in X-ray Bi- naries, ed. W. H. G. Lewin, J. van Paradijs, & E. P. J. van den Heuvel (Cambridge Univ. Press, Cambridge), 308 89
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UNIVERSITAT DE BARCELONA Departamen
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Per a la meva neboda Blanca, que va
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feina no presentada en aquesta tesi
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desfogar-nos conjuntament, per la s
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From the scientifical point of view
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Gràcies a la meva germana Nàdia,
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ii CONTENTS I Discovery and study o
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iv CONTENTS II A search for new mic
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vi CONTENTS
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viii Resum de la tesi d’Eddington
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x Resum de la tesi imprescindible p
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xii Resum de la tesi dels sistemes
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xiv Resum de la tesi un comportamen
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xvi Resum de la tesi MilliARC SEC 4
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xviii Resum de la tesi per poder de
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xx Resum de la tesi valors força s
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xxii Resum de la tesi 2. D’entre
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xxiv Resum de la tesi pano Alemán
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xxvi Resum de la tesi 3.3 Observaci
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xxviii Resum de la tesi habitual en
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xxx Resum de la tesi Per tant, si l
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xxxii BIBLIOGRAFIA
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2 Chapter 1. Introduction and backg
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10 Chapter 1. Introduction and back
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28 BIBLIOGRAPHY Lewin, W. H. G., va
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30 BIBLIOGRAPHY
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Chapter 2 Multiwavelength approach
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2.3. An interesting target in the s
Page 83 and 84: 2.4. The radio counterpart: NVSS J1
Page 101 and 102: 2.5. The optical/IR star: LS 5039 5
Page 111 and 112: 2.6. The X-ray counterpart: RX J182
Page 121 and 122: 2.7. The γ-ray counterpart: 3EG J1
Page 123 and 124: 2.7. The γ-ray counterpart: 3EG J1
Page 125 and 126: 2.8. A proposed scenario to explain
Page 127 and 128: Figure 2.23: Scenario where the mul
Page 133: 2.9. Conclusions 87 8. We have carr
Page 137 and 138: BIBLIOGRAPHY 91 Merck, M., Bertsch,
Page 139 and 140: Chapter 3 LS 5039 as a runaway micr
Page 141 and 142: 3.1. Positions and proper motions 9
Page 143 and 144: 3.1. Positions and proper motions 9
Page 145 and 146: 3.3. The past trajectory of LS 5039
Page 147 and 148: 3.4. SNR G016.8−01.1 101 DECLINAT
Page 149 and 150: 3.4. SNR G016.8−01.1 103 Normaliz
Page 151 and 152: 3.4. SNR G016.8−01.1 105 Galactic
Page 153 and 154: 3.5. The H i surroundings of LS 503
Page 155 and 156: 3.6. Discussion 109 experienced a h
Page 157 and 158: 3.6. Discussion 111 At this point w
Page 159 and 160: 3.7. Conclusions 113 6. Finally, th
Page 161 and 162: Bibliography Ankay, A., Kaper, L.,
Page 163 and 164: BIBLIOGRAPHY 117 Schaerer, D., de K
Page 165: Part II A search for new microquasa
Page 168 and 169: 122 Chapter 4. The cross-identifica
Page 176 and 177: 130 BIBLIOGRAPHY
Page 178 and 179: 132 Chapter 5. Radio and optical ob
Page 180 and 181: DECLINATION (J2000) DECLINATION (J2
Page 182 and 183: 136 Chapter 5. Radio and optical ob
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138 Chapter 5. Radio and optical ob
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148 BIBLIOGRAPHY
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150 Chapter 6. EVN and MERLIN obser
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166 BIBLIOGRAPHY
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General conclusions 171 Since each
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