arXiv (All)
open access
From spirals to rings: dust dynamics in gravitoturbulent protoplanetary discs after late infall
Substructures appear to be a common trait of all extended protoplanetary discs. They are found notably in discs still surrounded by ambient, possibly infalling material. In this study, we revisit the observational signatures of gravitational instability (GI) in the dust and gas emission of protoplan
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- Radiation Hydrodynamics of Self-gravitating Protoplanetary Disks II. Accretion, Migration, Spin, and Internal Structure of GI Fragments#1142286
- Gravito-turbulent bi-fluid protoplanetary discs#1146323
- Drift-dominated dust evolution. A multiwavelength analysis of dust rings in CY Tau and DoAr25#924752
- Drift-dominated dust evolution. A multiwavelength analysis of dust rings in CY Tau and DoAr25#920518
- Planet formation in chemically diverse and evolving discs II. Chemical fingerprints in planetary atmospheres#985159
Record · ID 997263
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Bring this data into your agent: Connect via MCP or API · 20 free credits to start · no card required
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive