Back to the Abstract

	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