arXiv (All)
open access
ELUCID. IX. Recovering the Substructures and History of the Coma Cluster
We employ constrained hydrodynamic simulations of the Coma galaxy cluster from the ELUCID project to study its substructures and assembly history. Our simulations accurately reproduce the global properties of Coma, including its position, virial mass, radius, and surrounding large-scale filaments. U
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
- Resolution to Galaxy Rotation Curves, Tully-Fisher, Radial Acceleration Relation, and Missing Satellites: Cosmological Coda V of the Principia Cybernetica#108956
- Baryonic assembly bias in X-ray-selected galaxy groups and clusters: insights from the Magneticum simulation#1011155
- GalSyn I: A Forward-Modeling Code for Synthetic Galaxy Observations from Hydrodynamical Simulations and First Data Release from IllustrisTNG#609890
- MACS: The evolution and properties of massive clusters of galaxies#639352
- Extragalactic Globular Cluster Systems: A new Perspective on Galaxy Formation and Evolution#639441
Record · ID 1048809
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