Early Planet Formation in Embedded Disks (eDisk). XXV. Inclination-Induced Minor-Axis Brightness Asymmetries Reveal Limited Dust Settling in Embedded Protostellar Disks

arXiv:2609.39501 · astro-ph.EP, astro-ph.SR · Submitted 2026-09-30 · Read on arXiv

astro-ph.EP, astro-ph.SR

Submitted: 2026-09-30

Updated: 2026-10-01

Code: https://github.com/dullemond/radmc3d-2.0

Terminology

• Core — 3× in this paper · explained in 2 episodes
• Streaming Instability — 3× in this paper · explained in 2 episodes
• Anti-correlation — 2× in this paper · explained in 3 episodes
• Aggregation — 1× in this paper · explained in 1 episode
• Magnetohydrodynamics (MHD) — 1× in this paper · explained in 3 episodes
• Markov Chain Monte Carlo — 1× in this paper
• National Science and Technology Council — 1× in this paper
• Trace — 1× in this paper · explained in 2 episodes

Sources

• Physical processes in protoplanetary disks

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