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Gràcies a la meva germana Nàdia, pels anys que hem viscut junts i per ser una excel·lent companya de pis durant els primers anys de tesi. De vegades encara trobo a faltar aquelles xerrades de diumenge explicant-nos la setmana. En fi, va ser important tenir-te al meu costat durant la difícil situació personal/professional dels primers dos anys de tesi sense beca. Gràcies també al Pau pels ànims i el suport. I finalment, l’agraïment més important. Gràcies Noemí. Gràcies per cuidar- me, per animar-me, per escoltar-me en els moments en que més ho necessito, per recolzar-me durant aquest llarg i dur estiu, per ser com ets i per estar sempre al meu costat.
Contents Resum de la tesi: Descobriment i estudi del microquàsar LS 5039 i una cerca de nous microquàsars vii 1 Introduction and background 1 1.1 X-ray binaries . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1 1.1.1 High mass X-ray binaries . . . . . . . . . . . . . . . . . . . . . 3 1.1.2 Low mass X-ray binaries . . . . . . . . . . . . . . . . . . . . . 6 1.1.3 Radio emitting X-ray binaries . . . . . . . . . . . . . . . . . . 8 1.2 Microquasars . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 10 1.2.1 Projection and special relativity effects . . . . . . . . . . . . . 12 1.2.2 Quasars and microquasars . . . . . . . . . . . . . . . . . . . . 16 1.2.3 Known microquasars . . . . . . . . . . . . . . . . . . . . . . . 17 1.2.4 Accretion disk and jet formation . . . . . . . . . . . . . . . . . 21 1.2.5 Black hole states and radio emission . . . . . . . . . . . . . . 22 1.3 Motivation of the thesis . . . . . . . . . . . . . . . . . . . . . . . . . 24 i
Page 1: UNIVERSITAT DE BARCELONA Departamen
Page 5: Per a la meva neboda Blanca, que va
Page 8 and 9: feina no presentada en aquesta tesi
Page 10 and 11: desfogar-nos conjuntament, per la s
Page 12 and 13: From the scientifical point of view
Page 16 and 17: ii CONTENTS I Discovery and study o
Page 18 and 19: iv CONTENTS II A search for new mic
Page 20 and 21: 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
Page 42 and 43: xxviii Resum de la tesi habitual en
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
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18 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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2.6. The X-ray counterpart: RX J182
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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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¡¢ ¢ ¢ ¡¢ £¤ ¡¢ ¤ ¢
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General conclusions 171 Since each
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