Our stellar evolution model for HD 49933.
|M/M⊙||R/R⊙||log g||Y 0||(Z/X)0||α||α ov||Age (My)||Teff (K)||log L/L⊙||X c||Y s||(Z/X)s||[Fe/H]|
Notes. The mass M, initial helium content Y0, metallicity (Z/X)0, core overshoot αov, and mixing length α are adjusted to reproduce the radius obtained by interferometry and the observed large and small separations.
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