ALMA Band 7 data on the faintest Lupus disks show compact gas structures explain weak CO emission without CO depletion and reveal no evidence for dust radial drift.
A.1: Visibility plots of observed and modeled visibilities, obtained withGALARIOby fitting a Gaussian profile to the millimeter emission
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Compact CO emission and no evidence of radial drift. ALMA observations of the faintest planet-forming disks in Lupus
ALMA Band 7 data on the faintest Lupus disks show compact gas structures explain weak CO emission without CO depletion and reveal no evidence for dust radial drift.