HAL (France)
open access
The CO snow line favours strong clumping by the streaming instability in protoplanetary discs with porous grains
Context: The radial drift and fragmentation of small dust grains in protoplanetary discs impedes their growth past centimetre sizes. Several mechanisms have been proposed to overcome these planet formation barriers, such as dust porosity or the streaming instability (SI), which is today regarded as
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