Protoplanetary Disks as (Possibly) Viscous Disks
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Peer-reviewed
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Abstract
Protoplanetary disks are believed to evolve on Myr timescales in a diffusive
(viscous) manner as a result of angular momentum transport driven by internal
stresses. Here we use a sample of 26 protoplanetary disks resolved by ALMA with
measured (dust-based) masses and stellar accretion rates to derive the
dimensionless
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1538-4357
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Science and Technology Facilities Council (ST/P000673/1)