arXiv (OAI Expanded)
open access
Second Generation Planet Formation in Post-AGB Discs - II: Dust Coagulation and Core Accretion
Observations have established that the circumbinary discs formed around post-asymptotic giant branch (post-AGB) binaries have striking similarities to protoplanetary discs around young stars. In this study, we examine the feasibility of the different stages of growth in the core accretion framework
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
- Investigating Variability in Long-lived Protoplanetary Disks (>10 Myr) using NEOWISE#1083444
- On the origin and survival of circumbinary planets in Post Common Envelope Binaries / Deepali Deepali ; Betreuer: Robi Banerjee#1145393
- Stability of circumbinary planets: the role of binary properties and migration scenarios#972083
- Dynamical Impacts of Accretion Streamers on Protoplanetary Disks#1119180
- Planetary migration in evolving planetesimal disks#204567
Record · ID 1084736
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