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166 BIBLIOGRAPHY
Chapter 7 Summary After a detailed analysis of our data, we show in Table 7.1 a summary of the results obtained after the VLA and optical observations presented in Chapt. 5, and the EVN+MERLIN observations reported in Chapt. 6. As can be seen, 1RXS J001442.2+580201 and 1RXS J013106.4+612035 are promising microquasar candidates. 1RXS J042201.0+485610 is probably of thermal nature due to its highly inverted spectrum at high radio frequencies, and we also note its extended appearance at optical wavelengths. 1RXS J062148.1+174736 is probably extragalactic due to the extended optical counterpart. 1RXS J072259.5−073131 displays a bent one-sided jet, which is a common property in blazars. Finally, the source 1RXS J072418.3−071508 is an already identified quasar. We note that none of the 6 sources studied here appears in the Third EGRET Catalog of high-energy γ-ray sources. We point out that 1RXS J072259.5−073131 is bright enough at radio wavelengths to attempt an H i absorption experiment, that could allow to determine if this source is galactic or not. In any case, optical spectroscopic observations of the first five sources are in progress for autumn 2002, to clearly unveil their galactic or extragalactic nature. Finally, the two sources belonging to Group 1 that have not been observed yet, namely 1RXS J181119.4−275939 and 1RXS J185002.8−075833 will be eventually studied in the future, together with Group 2 sources. 167
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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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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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Page 163 and 164: BIBLIOGRAPHY 117 Schaerer, D., de K
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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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Page 217 and 218: General conclusions 171 Since each
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