arXiv (All)
open access
ALMA2040: The High-Redshift Circumgalactic Medium. Imaging the fueling and feedback of galaxies in the early universe
Galaxies do not form in isolation, but rather as part of a wider interconnected web mediated at their interface by an extended gaseous atmosphere - the Circum-Galactic Medium (CGM). This dynamic and multiphase region is fed and shaped by gas inflows and mergers from the intergalactic medium and by f
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
- MUSE-ALMA Haloes XVI: a census of the condensed baryons in z~0.5 HI absorption-selected galaxies#1234484
- MEGATRON: Dwarf Galaxy Quenching in the Epoch of Reionization#1132389
- The RAdio Galaxy Environment Reference Survey (RAGERS) Evidence of an anisotropic distribution of submillimeter galaxies in the 4C 23.56 protocluster at z=2.48#1290960
- The star-forming past and quenching of brightest cluster galaxies in TNG-Cluster#1215729
- A model to mini-quench early galaxies by balancing stellar feedback and gas accretion#1013863
Record · ID 1357431
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