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26 Chapter 1. Introduction and background
Bibliography Blandford, R. D., & Königl, A. 1979, ApJ, 232, 34 Blandford, R. D., & Payne, D. G. 1982, MNRAS, 199, 883 Blandford, R. D., & Znajek, R. L. 1977, MNRAS, 179, 433 Corbel, S., Fender, R. P., Tzioumis, A. K., et al. 2000, A&A, 359, 251 Drake, S. A., A Brief History of High-Energy Astronomy, http://heasarc.gsfc.nasa.gov/docs/heasarc/headates/heahistory.html Fender, R. P. 2001, MNRAS, 322, 31 Fender, R. P. 2002, in Proc. of Relativistic Flows in Astrophysics, ed. A. W. Guth- mann, M. Georganopoulos, A. Marcowith & K. Manolakou, Lecture Notes in Physics, 589, 101 Fender, R. P., & Hendry, M. A. 2000, MNRAS, 317, 1 Fender, R. P., & Kuulkers, E. 2001, MNRAS, 324, 923 Fender, R. P., Southwell, K., & Tzioumis, A. K. 1998, MNRAS, 298, 692 Fomalont, E. B., Geldzahler, B. J., & Bradshaw, C. F. 2001, ApJ, 558, 283 Hartman, R. C., Bertsch, D. L., Bloom, S. D., et al. 1999, ApJS, 123, 79 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 Koide, S., Shibata, K., Kudoh, T., & Meier, D. L. 2002, Science, 295, 1688 27
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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
Page 22 and 23: viii Resum de la tesi d’Eddington
Page 24 and 25: x Resum de la tesi imprescindible p
Page 26 and 27: xii Resum de la tesi dels sistemes
Page 28 and 29: xiv Resum de la tesi un comportamen
Page 30 and 31: xvi Resum de la tesi MilliARC SEC 4
Page 32 and 33: xviii Resum de la tesi per poder de
Page 34 and 35: xx Resum de la tesi valors força s
Page 36 and 37: xxii Resum de la tesi 2. D’entre
Page 38 and 39: xxiv Resum de la tesi pano Alemán
Page 40 and 41: xxvi Resum de la tesi 3.3 Observaci
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Page 44 and 45: xxx Resum de la tesi Per tant, si l
Page 46 and 47: xxxii BIBLIOGRAFIA
Page 48 and 49: 2 Chapter 1. Introduction and backg
Page 56 and 57: 10 Chapter 1. Introduction and back
Page 74 and 75: 28 BIBLIOGRAPHY Lewin, W. H. G., va
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Page 79 and 80: Chapter 2 Multiwavelength approach
Page 81 and 82: 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
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2.7. The γ-ray counterpart: 3EG J1
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2.8. A proposed scenario to explain
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Figure 2.23: Scenario where the mul
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2.9. Conclusions 87 8. We have carr
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Bibliography Blandford, R. D., & K
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BIBLIOGRAPHY 91 Merck, M., Bertsch,
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Chapter 3 LS 5039 as a runaway micr
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3.1. Positions and proper motions 9
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3.1. Positions and proper motions 9
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3.3. The past trajectory of LS 5039
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3.4. SNR G016.8−01.1 101 DECLINAT
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3.4. SNR G016.8−01.1 103 Normaliz
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3.4. SNR G016.8−01.1 105 Galactic
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3.5. The H i surroundings of LS 503
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3.6. Discussion 109 experienced a h
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3.6. Discussion 111 At this point w
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3.7. Conclusions 113 6. Finally, th
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Bibliography Ankay, A., Kaper, L.,
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BIBLIOGRAPHY 117 Schaerer, D., de K
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Part II A search for new microquasa
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122 Chapter 4. The cross-identifica
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130 BIBLIOGRAPHY
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132 Chapter 5. Radio and optical ob
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DECLINATION (J2000) DECLINATION (J2
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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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