arXiv (OAI Expanded)
open access
Exploring the dynamics of the Coma galaxy cluster by mapping its X-ray emission line profiles with XRISM
The intracluster medium (ICM) in merging galaxy clusters exhibits turbulence and bulk flows. Unraveling these components is crucial not only for elucidating the geometry of the cluster mergers, but also for understanding the physics of magnetic field amplification and relativistic particle accelerat
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
- Baryonic assembly bias in X-ray-selected galaxy groups and clusters: insights from the Magneticum simulation#1011155
- CHEX-MATE: X-ray surface brightness discontinuities across a representative cluster sample#1071384
- Simulation Study of Binary Mergers of Galaxy Clusters I: Properties of Merger Shocks and Radio Emission#792682
- Simulation Study of Binary Mergers of Galaxy Clusters I: Properties of Merger Shocks and Radio Emission#788682
- Multi-branch classification of diffuse cluster radio emission from the LOFAR two-metre sky survey#800122
Record · ID 1160768
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