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1 Introduction
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2 A quick review of past work on Pop-III stars
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3 Nuclear network and nucleosynthesis
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4 General physical input of the stellar models
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5 General properties of the stellar tracks
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6 Low- and intermediate-mass models
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7 Massive models
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8 Surface chemical changes
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9 Might we ever detect primordial stars?
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Appendix A: Tables of evolutionary tracks
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Appendix B: Tables of isochrones
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References
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