arXiv (All)
open access
Measuring the magnetization profiles of galaxy groups and clusters
Magnetic fields are vital in determining the physical conditions of baryons in massive halos. They are, however, notoriously difficult to observe. This impacts problems from our understanding of galaxy formation, to the observed deficit in the amplitude of thermal Sunyaev-Zel'dovich (tSZ) power spec
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
- Constraints on the magnetic field in the hadronic scenario for the origin of the radio halo in the A1795 galaxy cluster#799011
- Constraints on the magnetic field in the hadronic scenario for the origin of the radio halo in the A1795 galaxy cluster#797596
- Baryonic assembly bias in X-ray-selected galaxy groups and clusters: insights from the Magneticum simulation#1011155
- The interplay between AGN photo-ionization, radio jet, and star formation in the z $\sim$ 3.5 radio galaxy 4C +03.24#1037542
- Towards robust simulations of the galactic dynamo: a cross-code comparison between Eulerian and Lagrangian schemes#1186622
Record · ID 1469316
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