Hints on the origins of particle traps in protoplanetary disks given by the Mdust – M⋆ relation

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Fig. 2

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Dust density distribution after 1 Myr of evolution for no traps (left panel), weak traps (middle panel), and strong traps (right panel), for the case of M_⋆ = 0.1M_⊙ and α = 10⁻³. Top panels: the disk mass is M_disk = 0.05 M_⊙. Bottom panels: the disk mass is M_disk = 0.05 M_⋆.

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