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Fig. 3
Pebble-isolation mass as a function of ∂lnP∕∂lnr of unperturbed discs with different surface density gradients. Steeper surface density slopes s result in more negative ∂lnP∕∂lnr values. All simulations have been performed for planets in discs with H∕r = 0.05, f = 0 and α = 0.001.
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