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114 Chapter 3. LS 5039 as a runaway microquasar
Bibliography Ankay, A., Kaper, L., <strong>de</strong> Bruijne, et al. 2001, A&A, 370, 170 Benaglia, P., & Cappa, C. E. 1999, A&A, 346, 979 Caswell, J. L., & Lerche, I. 1979, MNRAS, 187, 201 Claret, A., & Cunha, N. C. S. 1997, A&A, 318, 187 Claret, A., Giménez, A., & Cunha, N. C. S. 1995, A&A, 299, 724 Combi, J. A., Romero, G. E., & Benaglia, P. 1998, A&A, 333, L91 Combi, J. A., Romero, G. E., Benaglia, P., & Mirabel, I. F. 2001, A&A, 370, L5 Condon, J. J., Cotton, W. D., Greisen, E. W., et al. 1998, AJ, 115, 1693 Dauphole, B., & Colin, J. 1995, A&A, 300, 117 Dubner, G., Giacani, E., Reynoso, E., et al. 1999, AJ, 118, 930 Fich, M., Blitz, L., & Stark, A. A. 1989, ApJ, 342, 272 Forbes, D. 2000, AJ, 120, 2594 Green, D. A. 2000, A Catalog of Galactic Supernova Remnants, Mullard Radio Astronomy Observatory, Cambridge, England, UK (available on the World Wi<strong>de</strong> Web at http://www.mrao.cam.ac.uk/surveys/snrs/) Høg, E., Fabricius, C., Makarov, V. V., et al. 2000, A&A, 357, 367 Huthoff, F., & Kaper, L. 2002, A&A, 383, 999 115
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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
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2.4. The radio counterpart: NVSS J1
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2.5. The optical/IR star: LS 5039 5
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Page 109 and 110: 2.5. The optical/IR star: LS 5039 6
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 and 134: 2.9. Conclusions 87 8. We have carr
Page 135 and 136: Bibliography Blandford, R. D., & K
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: 3.7. Conclusions 113 6. Finally, th
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
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Page 178 and 179: 132 Chapter 5. Radio and optical ob
Page 180 and 181: DECLINATION (J2000) DECLINATION (J2
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Page 196 and 197: 150 Chapter 6. EVN and MERLIN obser
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164 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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