Surface gravity (see Eq. (1)) of stars with a normal helium surface mass fraction (Y ≃ 0.26) near their Eddington limit, as a function of their surface temperature, according to Eq. (9).
|Γe → 1||4.82||3.61||3.22||2.72||2.02|
|Γe = 0.9||4.86||3.66||3.27||2.77||2.07|
|Γe = 0.8||4.91||3.71||3.32||2.82||2.12|
|Γe = 0.7||4.97||3.77||3.38||2.88||2.17|
|Γe = 0.5||5.12||3.91||3.52||3.03||2.32|
|Γe = 0.3||5.34||4.13||3.75||3.25||2.54|
|Γe = 0.1||5.81||4.61||4.22||3.72||3.02|
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