Self-consistent curved dust wall models for T Tauri disks indicate that matching observed JHK colors requires millimeter grains lifted 0.5-3 scale heights above the midplane, implying high midplane turbulence.
Revisiting the viscous disk model and updated disk masses
3 Pith papers cite this work. Polarity classification is still indexing.
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SKA-Mid Band 5b continuum observations at 12.5 GHz will resolve disk substructures at ~0.05 arcsec to investigate their origin and role in planet assembly.
citing papers explorer
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Modeling the curved dust sublimation front in protoplanetary disks: a potential probe of midplane turbulence
Self-consistent curved dust wall models for T Tauri disks indicate that matching observed JHK colors requires millimeter grains lifted 0.5-3 scale heights above the midplane, implying high midplane turbulence.
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Substructures in Planet-Forming Disks with the SKAO
SKA-Mid Band 5b continuum observations at 12.5 GHz will resolve disk substructures at ~0.05 arcsec to investigate their origin and role in planet assembly.
- Chemistry and IR emission of acetylene in planet-forming regions of T Tauri disks. Impact of elemental abundances and dust properties