LAUSR

Dust growth and planet formation by disc fragmentation

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0 Published in 2025 at "Monthly Notices of the Royal Astronomical Society: Letters"

DOI: 10.1093/mnrasl/slaf096

Abstract: It is often argued that gravitational instability of realistic protoplanetary discs is only possible at distances larger than ∼50 au from the central star, requiring high disc masses and accretion rates, and that therefore disc… read more here.

Keywords: disc; disc fragmentation; dust growth;