Issue |
A&A
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
TP.
![]() |
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 -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 -enhanced
composition tracks.
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