Evolution of the habitable zone of low-mass stars - Detailed stellar models and analytical relationships for different masses and chemical compositions

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Fig. 10

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Left: relative errors on the distance R_i of the inner boundary of the 4 Gyr CHZ, as estimated from the analytical model in Eq. (9). Right: as in the left panel, but for the CHZ outer boundary R_o, as estimated from the analytical model in Eq. (10).

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