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Table 1

Stellar lifetimes (in Myr) of the models used in this paper.

Z = 0.004 Z = 0.008

M ZAMS / M t MS t RGB t He t EAGB τ t MS t RGB t He t EAGB τ

1.0 5771.4 2050.5 92.85 10.97 7925.7 6751.9 2521.0 104.48 10.37 9387.8
1.2 3141.2 966.74 94.45 9.32 4211.7 3600.5 1182.0 97.96 10.47 4890.9
1.5 1847.2 164.02 94.34 9.25 2114.8 2097.9 193.39 99.37 9.81 2400.5
1.6 1525.1 117.01 103.22 9.08 1756.6 1725.1 137.98 100.87 11.36 1975.3
1.8 1088.4 65.25 131.73 11.28 1296.7 1223.8 78.85 128.10 11.80 1442.6
2.0 812.67 27.46 199.22 11.36 1050.7 900.54 32.11 236.41 14.57 1183.6
2.6 410.03 8.59 82.06 4.07 505.1 448.03 9.96 106.62 6.74 571.4
3.0 286.74 5.23 50.58 2.34 344.9 309.24 5.93 60.20 3.71 379.1
4.0 145.00 2.12 20.48 1.15 168.8 152.27 2.33 23.40 1.25 179.3
5.0 88.23 1.15 11.4 0.59 101.4 90.83 1.24 12.18 0.69 104.9
6.0 60.07 0.71 7.54 0.34 68.6 60.98 0.75 7.75 0.41 69.9

Notes. Columns 2–5 and 7–10 give the duration of the central hydrogen burning, RGB, core-He burning, and early AGB phases, respectively, for the two chemical compositions. The last columns of each metallicity group summarize the age τ at the beginning of the TP-AGB.

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