Gravitational instabilities in a protosolar-like disc - II. continuum emission and mass estimates

MG Evans, John Ilee, TW Hartquist, P Caselli, L Szucs, SJD Purser, AC Boley, RH Durisen & JMC Rawlings
Gravitational instabilities (GIs) are most likely a fundamental process during the early stages of protoplanetary disc formation. Recently, there have been detections of spiral features in young, embedded objects that appear consistent with GI-driven structure. It is crucial to perform hydrodynamic and radiative transfer simulations of gravitationally unstable discs in order to assess the validity of GIs in such objects, and constrain optimal targets for future observations. We utilize the radiative transfer code LIME (Line...
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