Tidal dissipation in rotating low-mass stars
and implications for the orbital evolution of close-in planets
I. From the PMS to the RGB at solar metallicity
F. Gallet, E. Bolmont, S. Mathis, C. Charbonnel, and L. Amard
Column 1: Logarithm of the time in yr
Column 2: Stellar luminosity in solar luminosity
Column 3: Stellar effective temperature (K)
Column 4: Stellar radius in solar radius
Column 5: beta = Mass aspect ratio (M_core/M_*)
Column 6: alpha = Radius aspect ratio (R_core/Reff)
Column 7: Surface rotation rate of the star (days). Initial rotation = 1.4 days
Column 8: Logarithm of the frequency averaged tidal dissipation (see Eq. 1 of paper I)
Column 9: Logarithm of the modified equivalent quality factor (see Eq. 5 of paper I)
Column 10: Logarithm of the structural frequency-averaged tidal dissipation (see Eq. 3 of paper I)
Column 11: Logarithm of the structural modified equivalent quality factor (see Eq. 6 of paper I)