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Fig. 6
Pebble accretion efficiency for a 0.1 M⊕ planet at thelocation of the H2O iceline. Top panel: iceline around a 0.1 M⋆ mass star (hgas = 0.03, η = 10−3; qp = 3 × 10−6). Bottom panel: iceline of a solar mass star (hgas = 0.05, η = 3 × 10−3, and qp = 3 × 10−7).
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