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. 1

Hertzprung-Russell diagram for some models from the PMS to cooling WD stage. The masses of the models are (from right to left) 0.7 (black), 1.0 (red), 1.4 (green), 3.0 (blue), and 8.0 (magenta) in solar units. α_MLT = 1.84, [Fe/H] = 0.00.

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