Fig. 2
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Solar luminosity (in L⊙) as a function of time in Myr (see details of the solar model in Sect. 3.7). The horizontal dashed line is showing the current solar luminosity. Our gas release model starts at 5 Myr (vertical dotted line) when the proto-planetary disk dissipates and the sun’s luminosity is around 0.6 L⊙.
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