arXiv (All)
open access
Cosmic web stripping and starvation of low-mass filament galaxies in TNG50
Galaxy properties are known to correlate with their location within the cosmic web. However, the role of filaments remains poorly understood, particularly for low-mass galaxies, which are expected to be more sensitive to environmental effects. In this work, we use the TNG50-1 simulation to investiga
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
- Stellar bar occurrence in TNG50 and TNG100: disentangling environmental effects and assembly history at z = 0#1000296
- Galaxies in the first two billion years: Earlier formation and quenching with surface-density modulated star formation and feedback#1000033
- Disc-Based Estimation of the Local Dark Matter Density and Velocity Distribution in IllustrisTNG50#822579
- Validation of the Hybrid Bias Expansion model for the galaxy bispectrum#665821
- Validation of the Hybrid Bias Expansion model for the galaxy bispectrum#664321
Record · ID 1144810
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