Repositorio UNAB
metadata only
CC BY 4.0
The evolution of low-mass central galaxies in the vicinity of massive structures and its impact on the two-halo conformity
Indexación: Scopus.
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
- Galaxy-SMBH co-evolution in 2,435 DESI disk galaxies and merger-free BH growth in bulgeless disks#1037117
- Fractal structures and the large scale distribution of galaxies#639463
- Triaxiality of the Milky Way dark matter halo and the microlensing optical depth towards the Large Magellanic Cloud#986601
- Eliminating Dark Matter: Wave Geometry in the Time Field Model as an Alternative for Galactic Dynamics#721777
- Investigating the Young Stellar Populations and Hierarchies in Nearby Galaxies with the UVIT. III. Evidence for a Largest Scale of Correlated Stellar Structures and a Non-universal Fractal Dimension#821050
Record · ID 1405409
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