arXiv (All)
open access
Linear gas mass density: a unifying descriptor of Cosmic Filaments
Cosmic filaments connect the nodes of the large-scale web and are thought to harbour a substantial fraction of the low-z baryon budget, yet a physically motivated framework for organising their diverse gas properties has been lacking. Here we show that the linear mass density $Λ$ = M_gas/L_fil, meas
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
- Pinpointing the cosmic web between massive galaxy clusters I. The incidence of HI and OVI as WHIM tracers#1248130
- R(V) parameter of the dust extinction curve: mapping based on hot stars and connections to diffuse interstellar bands#1341932
- Interpreting the LZ 248 keV Event using Dark QCD#1051380
- Relocating the SIMP Miracle in the Axion Portal#998798
- Effects of temperature-dependent optical properties on the determination of interstellar dust masses#986309
Record · ID 1401481
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