Fig. 5
Irradiation tracks of eight randomly sampled G-type stars (identified by stellar mass 0.8–1.04 M⊙) where the median background radiation field satisfies the criterion of 2000 ≤ G0 ≤ 104. The green bar indicates the boundaries of this constraint. Incident FUV radiation field strength is measured on the ordinate in units of G0. The time resolution is 1 kyr.
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