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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 8.

SEDs of disk models with curved walls. The upper panels are models with ϵ = 0.001, ﹩\dot{M}=1\times 1{0}^{-8}{M}_{\odot }\,{{\rm{yr}}}^{-1}﹩, and zbig = 0.5H. Two inclinations are shown: ﹩\cos (i)=0.4﹩ (i = 66﹩\mathop{.}\limits^{{\unicode{x000b0}}}﹩4, upper left) and ﹩\cos (i)=0.9﹩ (i = 25﹩\mathop{.}\limits^{{\unicode{x000b0}}}﹩8, upper right). Both panels show the contribution from the star (yellow), the curved wall (blue), the disk (green), the accretion shocks (magenta), and the total (black). The lower panels show models with ﹩\cos (i)=0.5﹩, and two values of ϵ: 0.01 (lower left) and 0.0001 (lower right). The colors indicate zbig values: 0.1H (red), 2H (blue), and 3H (green), and the line style corresponds to ﹩\dot{M}=1\times 1{0}^{-8}{M}_{\odot }\,{{\rm{yr}}}^{-1}﹩ (solid) and ﹩\dot{M}=1\times 1{0}^{-9}{M}_{\odot }\,{{\rm{yr}}}^{-1}﹩ (dashed).

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