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Fig. D.1
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C/O as a function of R at 2.5 Myr for models with no trap (black) or a warm trap (red) in a 50 au disc around a 0.1 M⊙ star with an ionisation rate of 1.3 × 10−17 s−1. Vertical lines mark the location of the minimum gas density (’Gap location’) and the pressure maximum where dust accumulates (’Dust ring’).
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