Up: Age-luminosity relations for low-mass stars
Appendix A: Tables containing evolutionary data
The evolutionary properties for all evolutionary models
calculated. They are given as Tables A1-A24 (A1-A12 for the
(canonical) case "C'' without diffusion and A13-A24 for case "D'',
the one including diffusion in the same form as Table A1
(which is the table for the C-case composition
). The columns relate to:
- 1.
- age (in 109 years);
- 2.
-
;
- 3.
-
;
- 4.
- central helium abundance
or relative mass of the
hydrogen-exhausted core,
;
the switching between the two
quantities is easily recognizable by the jump from a number close to 1
to one of order 0.2;
- 5.
- surface helium abundance ;
- 6.
-
,
the location of the bottom of the convective
envelope in relative mass coordinate;
corresponds to a convective
envelope of thickness
or to a completely radiative
envelope. In a few cases, the very last model exhibits already a
convective shell in the helium flash region. In these cases, this column
gives the bottom of this inner convective region and the value listed is
of order 0.2 or smaller;
- 7.
- relative mass of the convective core,
.
The tables are an extract of the full evolutionary results,
such that sufficiently, but not too many time-steps are provided. They
contain the most important stages, like ZAMS, turn-off and tip of the
RGB. The complete set of data can be obtained from the authors on
request.
Tables A1-A24
Up: Age-luminosity relations for low-mass stars
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