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Article Contents
1 Introduction
2 Evolutionary models
3 Derivation of the wind contributions
4 Stellar yields as a function of ${\vec M}_{\boldmath {\mathsf i}}$, ${\vec Z}$, and ${\vec \alpha}$
5 Comparison with other calculations
6 Final remarks
References
Appendix A: Tables of stellar yields and planetary nebulae chemical abundances

Copyright ESO 2001
Published by EDP Sciences