arXiv (All)
open access
From relics to stripped systems: the environmental origin of compact galaxies
Compact galaxies represent a key population for understanding galaxy evolution, but the relative role of internal structure and environment in shaping their origin remains unclear. We aim to investigate how the abundance and quenching of compact galaxies depend on environment, and to determine wheth
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
- Halo mass, star formation, and morphology in galaxies: A morphology-dependent connection between halo environment and star formation activity#972670
- ALMA-JELLY II. Constraining the radial profiles of the quenching timescales in ram-pressure-stripped galaxies#1109533
- The CAVITY project - The spatially resolved star formation rate of galaxies in voids#284308
- KBSS-InCLOSE II: First Detailed Insights on the Inner CGM of Low-Mass $z\sim2.3$ Galaxies#1105393
- The Structural Abundance Crisis of Massive Galaxies in Current Cosmological Simulations#799146
Record · ID 1012281
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