arXiv (All)open access
Non-Thermal Pressure due to Gas Motions in the Intracluster Medium: Confronting XRISM/Resolve with TNG-Cluster Simulations
cosmology and nongalactic astrophysics, astrophysics of galaxies, high energy astrophysical phenomena
This document is indexed with metadata only — full text is not available in the archive for this record.
Open the official source ↗
Record · ID 985193
Retrieved via
Conceptio — every document is proof-bundled with source, license, and retrieval metadata.