A multi-fluid approach for polydisperse pebble accretion - From particles to fluids, establishing the multi-fluid framework

Open Access

Fig. 9

Pebble accretion rate for the 10 M_⊕ planet from Fig. 8 (blue solid line), and in the static gas disc scenario (blue dashed line), decomposed over the different pebble species. Overlaid in red is the original MRN-distribution, as depicted earlier in Fig. 5.

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