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Cited article:

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Forming giant planets around late-M dwarfs: Pebble accretion and planet–planet collision

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Can the giant planets of the Solar System form via pebble accretion in a smooth protoplanetary disc?

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Planet Mass Function around M Stars at 1–10 au: A Plethora of Sub-Earth Mass Objects

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Planetesimal Growth in Evolving Protoplanetary Disks: Constraints from the Pebble Supply

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The Astrophysical Journal 948 (2) 98 (2023)
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Monthly Notices of the Royal Astronomical Society 523 (3) 3348 (2023)
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N-body simulation of planetary formation through pebble accretion in a radially structured protoplanetary disk

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Centimeter-sized Grains in the Compact Dust Ring around Very-low-mass Star CIDA 1

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Efficient planet formation by pebble accretion in ALMA rings

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Rapid formation of massive planetary cores in a pressure bump

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