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Table 4:

Rotation velocity, effective temperature, and surface abundances of Li and Be predicted for the stellar models that are still on the main sequence at the age of IC 4651
M $V_{\rm ZAMS}$ $V_{\rm Age}$ $T_{\rm eff}$ A(Li) A(Be)
$(M_{\odot})$ (km s-1) (km s-1) (K)        
    1.2 Gyr 1.7 Gyr 1.2 Gyr 1.7 Gyr 1.2 Gyr 1.7 Gyr 1.2 Gyr 1.7 Gyr
1.3 50 19.4 16.9 6532 6507 2.05 1.51 1.02 0.77
  80 28.3 24.4 6535 6528 1.24 0.37 0.62 0.22
  110 36.2 30.9 6520 6483 0.47 -0.59 0.2 -0.29
1.35 50 30.3 27.6 6687 6663 2.69 2.33 1.26 1.10
  80 28.6 24.5 6683 6670 1.16 0.24 0.57 0.15
  110 36.6 31.5 6685 6676 0.43 -0.70 0.20 -0.35
1.4 50 42.7 41.4 6834 6762 3.24 3.22 1.41 1.41
  80 67.8 67.8 6824 6764 3.20 3.10 1.41 1.39
  110 96 95.2 6826 6781 3.12 2.94 1.39 1.33
1.5 50 40.5 37.5 7094 6857 3.23 3.18 1.41 1.40
  80 66.5 62.7 7174 6948 3.13 2.94 1.40 1.34
  110 92.2 87.8 7136 6900 2.97 2.66 1.35 1.21

Notes. Models by Charbonnel & Lagarde (in preparation). See text for more details.


Source LaTeX | All tables | In the text

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