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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 7.

SEDs of the curved wall plus star for various zbig values: 0.5H (blue), 1H (orange), 2H (green), and 3H (red). The stellar photosphere is shown in black. The disk model has M* = 0.5 M⊙ and ﹩\dot{M}=1\times 1{0}^{-8}{M}_{\odot }\,{{\rm{yr}}}^{-1}﹩, with ﹩\cos (i)=0.5﹩, for ϵ = 0.01 (solid) and ϵ = 0.0001 (dashed).

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