Dust and Gas Transport in Substructured Nonideal MHD Wind-Launching Disks with Embedded Planets

arXiv:2607.20158 · astro-ph.EP · Submitted 2026-08-15 · Read on arXiv

Chun-Yen Hsu, Zhi-Yun Li, Xiao Hu, Yisheng Tu, Min-Kai Lin

astro-ph.EP

Submitted: 2026-08-15

Updated: 2026-08-19

Comments: Accepted by MNRAS on 2026 July 20. 20 pages, 14 figures, animated versions of the figures are attached in the individual captures

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

Terminology

• Trace — 7× in this paper · explained in 2 episodes
• Angular Momentum Transport — 6× in this paper · explained in 3 episodes
• Core — 6× in this paper · explained in 2 episodes
• Accretion Flows — 4× in this paper · explained in 1 episode
• Abundance — 3× in this paper · explained in 1 episode
• Ambipolar Diffusion — 2× in this paper · explained in 1 episode
• Benchmark — 1× in this paper · explained in 2 episodes
• Magnetohydrodynamics (MHD) — 1× in this paper · explained in 3 episodes
• Metallicity — 1× in this paper · explained in 3 episodes

Sources

• Planet formation theory: an overview
• Rossby wave instability in weakly ionized protoplanetary disks. I. azimuthal or vertical B-fields
• Dust Clumping in Outer Protoplanetary Disks: the Interplay Among Four Instabilities
• Circumplanetary Disks are Rare around Planets at Large Orbital Radii: A Parameter Survey of Flow Morphology around Giant Planets

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