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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 9.

KDE maps of the observed dereddened JHK colors (blue region), with relative density isocontours shown at values of 9, 7.5, 6, 4.5, 3, and 1.5, from innermost (highest relative density) to outermost (lowest relative density). The colored symbols correspond to models with curved walls for different ﹩\cos (i)﹩ as indicated by the labels. The first row shows models with ϵ = 0.01 and the second row models with ϵ = 0.0001. The size of the symbol increases with ﹩\dot{M}﹩ and the color indicates the values for zbig. We show models for a 0.5 M, 1 Myr old star.

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