The efficiency of dust trapping in ringed proto-planetary discs
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Peer-reviewed
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Abstract
When imaged at high-resolution, many proto-planetary discs show gaps and
rings in their dust sub-mm continuum emission profile. These structures are
widely considered to originate from local maxima in the gas pressure profile.
The properties of the underlying gas structures are however unknown. In this
paper we present a method to measure the dust-gas coupling
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1365-2966
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European Commission Horizon 2020 (H2020) Marie Sk?odowska-Curie actions (823823)
Science and Technology Facilities Council (ST/N000927/1)