Modeling the curved dust sublimation front in protoplanetary disks: a potential probe of midplane turbulence

arXiv:2606.26232 · astro-ph.SR, astro-ph.EP · Submitted 2026-06-24 · Read on arXiv

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

University of Michigan · Universidad de Guadalajara · University of Michigan · Instituto de Astronomía-UNAM · Instituto de Radioastronomía y Astrofísica-UNAM · Universidad de Guadalajara

astro-ph.SR, astro-ph.EP

Submitted: 2026-06-24

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Abundance — 9× in this paper · explained in 1 episode
• Accretion Shock — 4× in this paper · explained in 1 episode
• Trace — 2× in this paper · explained in 2 episodes
• Adam — 1× in this paper · explained in 2 episodes
• Kavli Institute for Theoretical Physics — 1× in this paper
• Wide-field Infrared Survey Explorer — 1× in this paper

Sources

• Young Planets around Young Accreting Stars: I. Migration and Inner Stalling Orbits
• Models of Accretion Disks around Young Stars
• Demographics of young stars and their protoplanetary disks: lessons learned on disk evolution and its connection to planet formation

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