arXiv (OAI Expanded)
open access
Atomic diffusion in metal poor stars. The influence on the Main Sequence fitting distance scale, subdwarfs ages and the value of Delta Y/DeltaZ
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 impact of hot mode accretion and angular momentum conservation on metallicity gradients of galactic discs#819164
- The impact of hot mode accretion and angular momentum conservation on metallicity gradients of galactic discs#809172
- iPTF 16hgs: A Double-peaked Ca-rich Gap Transient in a Metal-poor, Star-forming Dwarf Galaxy#491880
- Shocks and Metallicity Gradients in Normal Star-Forming Galaxies#497509
Record · ID 639370
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