arXiv (All)
open access
The Star Formation Histories of Different Components of M31's Halo from Photometric Estimates of Fe and $α$ Abundances
We present the chemical-abundance distributions and star-formation histories of the M31 halo components using photometric Fe and $α$ abundance estimates derived from the PAndAS broad-band $g$ and $i$ filters and the Subaru/HSC $NB515$ narrow-band filter. We selected about 76,400 candidate M31 giant
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
- Low-Metallicity Star Formation Survey in Sh2-284 (LZ-STAR): The Core Mass Function#1062971
- A Theoretical Study of the Stellar Parameters and Surface Nucleosynthesis of the Extremely Metal-Poor RGB Giant BD$-18^{\circ}$5550 - Part I: Effects of $α$-enhancement and Internal Mixing#996694
- Planetary Accretion Is Less Frequent in Wide Binaries: Evidence from Metal-Enriched White Dwarfs in DESI DR1#999484
- Internal Structure, Not Environment, Shapes Metallicity Gradients in Low-Mass Galaxies from MaNGA#1144656
- Turbulent gas-rich discs at high redshift: the origin of early massive stellar bars#925623
Record · ID 1389861
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