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Cited article:

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The role of density perturbation on planet formation by pebble accretion

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Efficient planet formation by pebble accretion in ALMA rings

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Increased isolation mass for pebble accreting planetary cores in pressure maxima of protoplanetary discs

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Giant planet formation at the pressure maxima of protoplanetary disks

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Thermal torque effects on the migration of growing low-mass planets

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