arXiv (OAI Expanded)
open access
The Structural Abundance Crisis of Massive Galaxies in Current Cosmological Simulations
The internal structure of galaxies encodes the complex baryon cycle driven by gas accretion, star formation, and feedback, together with secular evolution and environmentally driven processes such as mergers and tidal interactions. We present a population-level census of massive nearby galaxies ($\l
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 Structural Abundance Crisis of Massive Galaxies in Current Cosmological Simulations#799146
- Unveiling the population of massive quenched galaxies at $z\ge2$ in the COLIBRE simulations - II. The role of AGN feedback and environment on their emergence#999246
- Lower central dark matter densities in nearby galaxies than predicted by simulations#1122747
- The Low-Mass Baryon Cycle in QUEST Dwarf Galaxies I: Sample definition and first results#616921
- The Low-Mass Baryon Cycle in QUEST Dwarf Galaxies I: Sample definition and first results#616421
Record · ID 797723
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