arXiv (All)
open access
Metal-Poor Stars as Metal-Rich Impostors via Planet Engulfment
Planet engulfment leads to planetary mass accretion and angular momentum deposition into the stellar envelope. This study uses MESA models to investigate the long-term impact of engulfment on stellar metallicity and rotational velocity, as well as the effect of rotational mixing on metal enrichment.
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
- In-Situ Star Formation in a Thick Disk: A Model for Metal Enrichment of Mrk 573#1063259
- The elderly among the oldest: new evidence for extremely metal-poor RR Lyrae stars#196908
- Abundances in Very Metal-Poor Stars#639328
- Wind properties of Wolf-Rayet stars at low metallicity: Sk41 (SMC)#639322
- Extremely metal-poor stars in the Fornax and Carina dwarf spheroidal galaxies#315148
Record · ID 1077103
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