Table B.1
Results obtained with BONNSAI for stars for which atmospheric parameters and He, C, N, O abundances can be reproduced with Bonn models when Teff, log gC, vsin i, y, log ϵ(C), log ϵ(N), and log ϵ(O) are given as input to BONNSAI.
Star | BD +34° 1058 | BD +60° 594 | HD 14434 | HD 14442 | HD 15137 | HD 41161 | ||||||||||||||
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Mini (M⊙) |
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Mact (M⊙) |
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log L (L⊙) |
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Age (Myr) |
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τ MS |
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vini (km s-1) |
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vsin i (km s-1) | ![]() |
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i (°) | 90.0 | 53.1 | 77.3 | 74.9 | 74.6 | 75.4 | ||||||||||||||
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log ϵ(C) | ![]() |
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log ϵ(N) | ![]() |
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log ϵ(O) | ![]() |
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Star | HD 46056 | HD 46485 | HD 52533 | HD 66811 | HD 69106 | HD 74920 | ||||||||||||||
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Mini (M⊙) |
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Mact (M⊙) |
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log L (L⊙) |
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Age (Myr) |
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τ MS |
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vini (km s-1) |
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vsin i (km s-1) | ![]() |
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i (°) | 76.5 | 90.0 | 52.6 | 66.4 | 75.6 | 58.0 | ||||||||||||||
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log ϵ(C) | ![]() |
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log ϵ(N) | ![]() |
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log ϵ(O) | ![]() |
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Star | HD 117490 | HD 124979 | HD 149757 | HD 175876 | HD 191423 | HD 192281 | ||||||||||||||
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Mini (M⊙) |
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Mact (M⊙) |
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log L (L⊙) |
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Age (Myr) |
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τ MS |
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vini (km s-1) |
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vsin i (km s-1) | ![]() |
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i (°) | 76.6 | 62.7 | 76.8 | 74.6 | 77.5 | 74.6 | ||||||||||||||
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log ϵ(C) | ![]() |
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log ϵ(N) | ![]() |
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log ϵ(O) | ![]() |
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Star | HD 203064 | HD 210839 | HD 228841 | |||||||||||||||||
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Mini (M⊙) |
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Mact (M⊙) |
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log L (L⊙) |
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Age (Myr) |
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τ MS |
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vini (km s-1) |
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vsin i (km s-1) | ![]() |
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i (°) | 75.4 | 73.0 | 75.6 | |||||||||||||||||
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log ϵ(C) | ![]() |
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log ϵ(N) | ![]() |
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log ϵ(O) | ![]() |
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Notes. Observed values of Paper I are indicated between parentheses. Mini and Mact are the initial and current stellar masses, respectively, L is the stellar bolometric luminosity, τMS is the fractional MS age, i is the inferred stellar inclination from the actual and projected rotational velocities given by BONNSAI, and vini is the initial rotational velocity. Errors from BONNSAI correspond to 1σ, except for values flagged with † for which the errors are slightly larger than 1σ.
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