arXiv (All)
open access
Where planetary solids survive sublimation around young and hot white dwarfs
All observed planetary systems orbiting single white dwarfs have lived through the hot stellar transition from an asymptotic giant branch star. In this post-nebular transition period, the initial conditions for planetary system evolution throughout white dwarf cooling are established. The hottest ($
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
- Where planetary solids survive sublimation around young and hot white dwarfs#809851
- Pristine composition or size evolution: Can current dust models reproduce emissivities observed in nearby protostars?#1079617
- The Effect of X-Ray and Accretion Variability on Mid-Infrared Lines in the Young Disk-Bearing Binary DQ Tau#974944
- The Dense, Rocky Core of Haumea Revealed by Satellite Dynamics#1130879
- Mass-Orbital Period Distribution of Massive White Dwarfs Formed Through Stable Mass Transfer#1069813
Record · ID 819847
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