arXiv (OAI Expanded)
open access
Magnetohydrodynamics of charged interstellar dust. Multifluid models and study of the linear modes
Interstellar grains play key roles in star and planet formation, including the coupling of the gas to the magnetic field during the protostellar collapse. These roles depend on the local grain size distribution, which requires a multifluid treatment of charged dust. We aim to understand the fundamen
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
- Magnetohydrodynamics of charged interstellar dust. Multifluid models and study of the linear modes#818766
- A Split-Flux Method for Dust-Gas Two-Fluid Simulations from Strong to Weak Coupling#1063976
- Rock magnetic of sediment core MD95-2040#145298
- Testing various assumptions for radiolysis, non-diffusive chemistry, and chemical desorption in cold cores#1120537
- The influence of galaxy mergers, black-hole growth, and gas processes on the evolution of the stellar mass-gas metallicity relation of galaxies in different cosmic environments#985007
Record · ID 808774
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