arXiv (All)
open access
Halo mass, star formation, and morphology in galaxies: A morphology-dependent connection between halo environment and star formation activity
Understanding the mechanisms responsible for quenching star formation in galaxies requires disentangling the roles of internal structure and large-scale environment. We investigate how galaxy morphology and specific star formation rate (sSFR) relate to the typical masses of host dark-matter halos (D
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
- Starbursts hiding in the main sequence: a pathway toward quenching?#1143693
- Path Measures for Stochastic Galaxy Formation on Layered Halo Graphs#1076834
- Dark Matter Halo Tumbling Induced by Torques from Massive Mergers#822222
- From relics to stripped systems: the environmental origin of compact galaxies#1012281
- The role of outflows and star formation efficiency in the evolution of early-type cluster galaxies#639550
Record · ID 972670
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