arXiv (All)
open access
Understanding the formation of alpha-Fe bimodality in the Milky Way using constrained cosmological simulations of the Local Group
We use a novel suite of constrained cosmological simulations of the Local Group to investigate the formation of alpha--Fe bimodalities in stellar discs of Milky Way analogues. In agreement with past studies using the Auriga model, we show that in our simulations the high-alpha sequence forms in a me
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
- The Structure of Dark Matter Haloes in Cosmological Simulations#387507
- X-ray and Radio Analysis of Abell 1644: Constraints on Cluster Dynamics#1128504
- Euclid preparation. The shape of halo profiles in $Λ$CDM and non-standard cosmologies#927055
- Dynamical Evolution of The Open Clusters Collinder 110 and NGC 2477#1115881
- PIANISTpy: A JAX-based Python package for velocity-anisotropic astrophysical equilibrium models#1412999
Record · ID 1411960
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