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Table 2

Properties of the 20 M model computed with different codes, without rotation, and evaluated at four different evolutionary phases.

Phase STERN2 Geneva FRANEC Padova MESA STAREVOL

Xc = 0.5
Teff(K) 33 522 33 758 33 709 32 538 33 011 33 365
4.764 4.733 4.736 4.747 4.745 4.733
age (Myr) 3.598 3.745 4.079 4.279 4.073 3.963

TAMS3
Teff(K) 24 630 29 297 28 094 25 972 28 733 27 902
5.096 5.001 5.036 5.045 5.007 4.995
age (Myr) 8.173 7.819 9.085 9.100 8.598 8.535

ZAHeMS
Teff(K) 5388 24 014 27 382 15 657 23 200 24 259
4.987 5.025 5.012 5.044 5.042 5.015
age (Myr) 8.185 7.828 9.088 9.111 8.610 8.541

TAHeMS3
Teff(K) 3753 3817 3550 3702 3462
5.050 5.206 5.090 5.049 5.027
age (Myr) 8.713 9.690 9.820 9.530 9.748

Notes. When the central H mass fraction is 0.5 (Xc = 0.5); at the terminal age main sequence (TAMS); at the zero age helium burning main sequence (ZAHeMS); at the terminal age helium burning main sequence (TAHeMS).

(2)

For the STERN grid, the data available stop at the beginning of the core He burning phase.

(3)

The TAMS and TAHeMS are defined as the points where the mass fraction of H (resp. He) is lower than 10-5.

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