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Modeling the Curved Dust Sublimation Front in Protoplanetary Disks: A Potential Probe of Midplane Turbulence

  • Authors: Ezequiel Manzo-Martínez, Ramiro Franco Hernández, Nuria Calvet, Jesús Hernández, Paola D'Alessio, Rosa M. Torres

Ezequiel Manzo-Martínez et al 2026 The Astrophysical Journal 1006 .

  • Provider: AAS Journals

Caption: Figure 10.

Distributions of ﹩\mathrm{log}(\epsilon )﹩ (upper left), ﹩\dot{M}﹩ (upper right), ﹩\cos (i)﹩ (lower left), and zbig (lower right) of the disk models that populate the region defined by the two innermost relative density isocontours (with KDE values 9 and 7.5) of the observations.

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