Theoretical tidal evolution constants for stellar models from the pre-main sequence to the white dwarf stage - Apsidal motion constants, moment of inertia, and gravitational potential energy

Open Access

Fig. 4

Time evolution of the function Γ(mass, EOS) for a model with initial mass of 7.00 M_⊙ evolving from the PMS to the WD stage, α_MLT=1.84, f_ov = 0.016, [Fe/H]=0.00. The red line represents Γ(mass, EOS), while the black line indicates the total thermal power from PP and CNO (excluding neutrinos) and the blue line indicates the total thermal power from triple-α (also excluding neutrinos). The nuclear power ϵ_N is in logarithmic scale.

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