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

Copyright ESO 2001
Published by EDP Sciences