arXiv (All)
open access
Tracing M22's origins: Spatial and chemical constraints on its formation history
Globular clusters (GCs) are well known to host stellar populations characterized by light-element variations. A subset of Galactic GCs, beyond such 'canonical' populations, contains an additional group enriched in iron, s-process elements, and total C+N+O abundance (i.e., the anomalous stars). We co
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
- Hint of bimodal Mg-Al anticorrelation in the metal-poor Globular Cluster NGC 4372#927655
- Low-Metallicity Star Formation Survey in Sh2-284 (LZ-STAR): The Core Mass Function#1062971
- Open Clusters as Laboratories for Cool Star Evolution: Highlights from the Cool Stars 23 Splinter Session#999316
- The dynamical environment of the high-mass star-forming region G28.288$-$0.364#1014768
- Ongoing Large Surveys for Metal-Poor Stars in the Galactic Halo#639367
Record · ID 996589
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