Size-sorting dust grains in the surface layers of protoplanetary disks
Size-sorting dust grains in the surface layers of protoplanetary disks
Context. The shape of dust emission features measured from protoplanetary disks contains information about the typical size of the dust particles residing in these disks. A flattened 10 μm silicate feature is often interpreted as proof that grain growth has taken place, while a pointy feature is taken as evidence …