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Table 3.

Properties of non-rotating stellar models at the end of core carbon burning.

MZAMS log(L/L) R Mfinal Menv MHe MCO
(M) (R) (M) (M) (M) (M)
9 4.52 418 8.94 6.47 2.47 1.37
10 4.63 480 9.95 7.11 2.84 1.59
11 4.72 536 10.95 7.75 3.21 1.80
12 4.80 586 11.95 8.44 3.51 2.02
13 4.87 640 12.92 9.02 3.90 2.29
14 4.94 694 13.88 9.57 4.31 2.59
15 5.00 746 14.84 10.14 4.69 2.89
16 5.07 804 15.85 10.66 5.20 3.27
17 5.12 850 16.80 11.24 5.56 3.58
18 5.15 879 17.64 11.82 5.82 3.83
19 5.20 932 18.51 12.25 6.26 4.23
20 5.25 1000 19.26 12.45 6.81 4.71
21 5.31 1070 19.93 12.55 7.38 5.22
22 5.35 1124 20.61 12.72 7.88 5.68
23 5.37 1149 21.22 12.84 8.38 6.14
24 5.42 1227 21.63 12.66 8.97 6.68
25 5.46 1294 21.96 12.43 9.53 7.20
26 5.49 1322 22.34 12.31 10.03 7.66
27 5.52 1387 22.52 11.94 10.58 8.16
28 5.55 1441 22.78 11.70 11.08 8.63
29 5.59 1508 22.72 11.07 11.64 9.15
30 5.62 1564 22.68 10.50 12.18 9.65

Notes. Columns: (1) Initial mass; (2) logarithm of the stellar luminosity; (3) stellar radius; (4) total final mass; (5) hydrogen-rich envelope mass; (6) helium-core mass; (7) carbon-oxygen core mass.

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