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. 1

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Temporal evolution of the inner d_i and outer d_o boundaries of the HZ for host stars of M = 0.70 M_⊙ (left panel) and M = 1.10 M_⊙ (right panel) for Z = 0.005, Y = 0.2585 (i.e. ΔY/ ΔZ = 2), and T_o = 169 K. The HZ is the region between the two curves. The dashed lines mark the distance for which the HZ lasts longer.

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