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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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4 Chapter 1. Introduction and backg
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6 Chapter 1. Introduction and backg
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8 Chapter 1. Introduction and backg
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10 Chapter 1. Introduction and back
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12 Chapter 1. Introduction and back
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14 Chapter 1. Introduction and back
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16 Chapter 1. Introduction and back
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18 Chapter 1. Introduction and back
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20 Chapter 1. Introduction and back
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22 Chapter 1. Introduction and back
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24 Chapter 1. Introduction and back
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26 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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2.4. The radio counterpart: NVSS J1
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2.4. The radio counterpart: NVSS J1
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2.4. The radio counterpart: NVSS J1
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2.4. The radio counterpart: NVSS J1
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2.4. The radio counterpart: NVSS J1
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2.4. The radio counterpart: NVSS J1
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2.4. The radio counterpart: NVSS J1
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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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2.5. The optical/IR star: LS 5039 5
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2.5. The optical/IR star: LS 5039 5
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2.5. The optical/IR star: LS 5039 6
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2.5. The optical/IR star: LS 5039 6
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2.6. The X-ray counterpart: RX J182
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2.6. The X-ray counterpart: RX J182
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2.6. The X-ray counterpart: RX J182
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2.6. The X-ray counterpart: RX J182
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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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2.8. A proposed scenario to explain
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2.8. A proposed scenario to explain
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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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- Page 147 and 148: 3.4. SNR G016.8−01.1 101 DECLINAT
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- 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
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- Page 217 and 218: General conclusions 171 Since each