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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 3.

Visualization of the shape of the curved wall model as seen at an inclination ﹩\cos (i)=0.4﹩. The parameters are ﹩\dot{M}=1\times 1{0}^{-8}\,{M}_{\odot }\,{{\rm{yr}}}^{-1}﹩, ϵ = 0.01, and zbig = 0.1H, for a 0.5 M⊙ star. Note that the lower wall is not visible except through the central hole. The star is shown at the center.

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