EDP Sciences
Free Access
Volume 508, Number 3, December IV 2009
Page(s) 1343 - 1358
Section Stellar structure and evolution
DOI https://doi.org/10.1051/0004-6361/200912043
Published online 19 November 2009

Online Material

Appendix A: Evolution up to the first TP

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

\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).

Open with DEXTER

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.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.