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Appendix A: Evolution up to the first TP

Table A.1:   Solar-scaled metallicity models from the ZAMS until the 1 $^{{\rm st}}$ TP.

\begin{figure} \par\includegraphics[angle=90,scale=0.3]{12043figA1a.ps}\includeg... ...12043figA1e.ps}\includegraphics[angle=90,scale=0.3]{12043figA1f.ps} \end{figure} Figure A.1:

Main sequence lifetimes ( left) and core mass at the first thermal pulse ( right) for three chemical compositions with Z=0.004, 0.008, 0.02 ( from top to bottom) of our models (crosses) in comparison with literature values from Karakas (2003, K03), Vassiliadis & Wood (1993, VW93), and Miller-Bertolami (private communication, 2008, MB08).

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Table A.2:   Same as for Table A.1 but for the $\alpha $-enhanced metallicity models.

Appendix B: Summary of AGB properties

Table B.1:   Same as Table 4, but for mixtures I and II (Table 1) with Z=0.04.

Table B.2:   Same as Table 4, but for mixtures V and VI (Table 1) with Z=0.008.

Table B.3:   Same as Table 4, but for mixtures VII and VIII (Table 1) with Z=0.004.

Table B.4:   Same as Table 4, but for mixtures IX and X (Table 1) with Z=0.0005.

Appendix C: Post-AGB evolution

Table C.1:   Post-AGB evolution for all models with solar-scaled metal distributions computed through this phasea.

Table C.2:   As Table C.1, but for the $\alpha $-enhanced composition tracks.