arXiv (All)
open access
A Splashback-like Feature of Central Galaxies in Galaxy Clusters
We investigate a splashback-like feature in the outer region of central galaxies (CGs) in clusters. This feature is detected as a "dip" in the radial slope of the CG surface brightness, derived through the stacking of Dark Energy Survey data of over 4000 galaxy clusters in the redshift range of 0.2
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
- Quantifying the decline in CO(2-1) intensity around PHANGS-HST star clusters: Constraints on molecular gas dispersal, stellar feedback, and cluster formation efficiency#1115794
- A complete redshift sample of galaxies#304074
- Lower central dark matter densities in nearby galaxies than predicted by simulations#1122747
- The molecular gas of four ram pressure stripped galaxies in the core of the Hydra I cluster#1062583
- Tidal Tails of Galactic Open Clusters: A Review of Methods, Evidence, and Sources of Disagreement#1035559
Record · ID 821726
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