Revisiting Kepler-444 - II. Rotational, orbital, and high-energy fluxes evolution of the system

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Fig. 6

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Evolution of the EUV and X-ray luminosity (solid and dashed line, respectively) computed using Eqs. (7) and (8) for the super-slow rotating case (Ω_in = Ω_⊙). The verticalline indicates the age of the system.

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