arXiv (All)
open access
Evidence of galaxy cluster rotation and intrahalo gas motions in the cosmic microwave background
We report the first robust evidence for the rotational kinematic Sunyaev-Zel'dovich (rkSZ) effect: the dipolar signal produced by the Thomson scattering of cosmic microwave background (CMB) photons off intracluster gas in dynamically active systems (including rotations and mergers). By combining CMB
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
- Stellar structures, molecular gas, and star formation across the PHANGS sample of nearby galaxies (Corrigendum)#333843
- Internal Structure, Not Environment, Shapes Metallicity Gradients in Low-Mass Galaxies from MaNGA#1144656
- The Neutral Hydrogen Gas Content of Star-forming and Quiescent S0 Galaxies#1064574
- ALMA High-J CO Spectroscopy of High-Redshift Galaxies. I. An Archive-based Catalog of CO Spectral Line Energy Distributions#1012137
- Dark Energy Survey Year 1 results: cross-correlation redshifts – methods and systematics characterization#1358153
Record · ID 1344484
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