Fig. E.1
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Timescales for ionization tion (red), leaving the disk tleave (orange), and stellar wind collisions with CO thit (blue) Vs distance to the gas. The fiducial model labeled as the “young system” has M⋆ = 1M⊙, υsw = 100 km/s, and Ω⋆ = 10 Ω⋆. The timescale tion for SW protons is shown for a young system but it is always an order of magnitude greater than thit.
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