arXiv (All)
open access
The Magnetized Universe: From planet-forming disks to the high-redshift universe
The interstellar medium (ISM) is magnetized at all scales and phases in our Galaxy and other galaxies across the Universe. Spectro-polarimetric millimetre observations are essential to probe the role of the interstellar magnetic fields in the dynamics of the cold universe, and how this affects the s
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
- A COSMOLOGICAL HIGH-REDSHIFT OBSERVATIONAL SURVEY WITH ATLAST: redshift, BAO, dusty star-forming galaxies, and the Hubble tension in critical-propositional dialogue with the Theory of Objectivity#319516
- Cross-correlation of CMB Polarization Lensing with High-z Submillimeter Herschel-ATLAS Galaxies#784309
- Microwave-Induced Optomagnetism in High-Temperature Superconductors#819147
- Microwave-Induced Optomagnetism in High-Temperature Superconductors#809155
- The dominant role of dark matter halo in quenching central galaxies#1013482
Record · ID 1386571
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