| Preface |
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vii | |
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Meteoritic Presolar Grains and Their Significance |
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1 | (24) |
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Presolar isotopic signatures and their carriers |
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3 | (5) |
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The discovery of presolar stellar grains |
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8 | (2) |
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Meteorites carrying stellar grains |
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10 | (1) |
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11 | (7) |
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13 | (1) |
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14 | (1) |
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14 | (2) |
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16 | (1) |
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17 | (1) |
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17 | (1) |
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New information from presolar grains |
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18 | (6) |
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Stellar evolution, nucleosynthesis and mixing |
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18 | (2) |
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Physical and chemical properties of the gas around stars and supernovae |
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20 | (2) |
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The interstellar medium, molecular clouds and early solar system |
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22 | (2) |
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24 | (1) |
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24 | (1) |
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Basics of Stellar Nucleosynthesis |
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25 | (34) |
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Hydrogen burning, and the life of most stars |
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27 | (9) |
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29 | (3) |
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The CNO, NeNa and MgAl cycles |
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32 | (4) |
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Helium burning, and the evolution of stars of low mass |
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36 | (3) |
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The α process: C, Ne and O burnings, and the evolution of stars of high mass |
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39 | (1) |
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The e process: Si burning, and supernova explosions |
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40 | (5) |
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The production of elements heavier than Fe |
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45 | (12) |
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49 | (2) |
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51 | (5) |
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56 | (1) |
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57 | (2) |
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Laboratory Analysis of Presolar Grains |
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59 | (18) |
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The isolation of diamond, graphite and SiC grains |
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59 | (3) |
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Looking at presolar grains |
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62 | (1) |
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Isotopic measurements with mass spectrometers |
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63 | (8) |
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65 | (1) |
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Secondary Ion Mass Spectrometry (SIMS) |
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65 | (3) |
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The advent of Resonant Ionization Mass Spectrometry (RIMS) in trace element analysis |
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68 | (3) |
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Location and analysis of rare types of presolar grains |
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71 | (3) |
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74 | (1) |
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75 | (2) |
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The Origin of Presolar SiC Grains |
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77 | (36) |
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Classification of SiC grains on the basis of their C, N and Si compositions |
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77 | (4) |
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Where did mainstream presolar SiC grains come from? |
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81 | (7) |
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Theoretical modelling of AGB and C(N) stars |
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83 | (5) |
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Carbon and nitrogen in mainstream SiC grains and in AGB stars |
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88 | (6) |
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The Ne-E(H) anomalous component |
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94 | (4) |
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98 | (1) |
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The puzzle of the silicon isotopic composition of mainstream SiC grains |
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99 | (6) |
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Titanium isotopic composition of mainstream SiC grains |
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105 | (3) |
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A, B, X, Y and Z: The minor SiC grains populations |
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108 | (3) |
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108 | (1) |
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109 | (1) |
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110 | (1) |
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111 | (2) |
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Heavy Elements in Presolar SiC Grains |
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113 | (38) |
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Modelling the s process in AGB stars |
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114 | (12) |
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The neutron source in AGB stars |
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115 | (2) |
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The production of a 13C pocket |
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117 | (4) |
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121 | (2) |
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The neutron flux in the 13C pocket |
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123 | (1) |
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The neutron flux in the thermal pulse |
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124 | (2) |
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SiC grain data and the s process in AGB stars |
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126 | (16) |
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Class I: Isotopic ratios involving p-only and r-only isotopes |
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126 | (4) |
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Class II: Isotopic ratios involving isotopes in local equilibrium |
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130 | (2) |
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Class III: Isotopic ratios involving isotopes with magic neutron numbers |
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132 | (5) |
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Class IV: Isotopic ratios involving isotopes depending on branchings |
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137 | (4) |
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Class V: Isotopic ratios involving isotopes produced by radioactive decay |
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141 | (1) |
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The heavy noble gases: Kr and Xe |
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142 | (5) |
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147 | (4) |
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Diamond, Graphite and Oxide Grains |
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151 | (14) |
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151 | (3) |
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154 | (3) |
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157 | (5) |
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162 | (3) |
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165 | (8) |
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Appendix B Solutions to Exercises |
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173 | (10) |
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173 | (1) |
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173 | (2) |
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175 | (2) |
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177 | (2) |
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179 | (2) |
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181 | (2) |
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Appendix C Selected Books and Reviews for Quick Reference |
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183 | (2) |
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183 | (1) |
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C.2 Stellar evolution and nucleosynthesis |
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183 | (1) |
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C.3 AGB stellar evolution and nucleosynthesis |
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184 | (1) |
| Bibliography |
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185 | (22) |
| Index |
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207 | |