Turbulent viscosity in line-driven stellar winds
astro-ph.SR
Submitted: 2026-10-06
Updated: 2026-10-06
Comments: 17 pages, 10 figures. Accepted for publication in The Astrophysical Journal
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Quasi-Keplerian Be-Star Disks with Mimicking Viscosity
- A Note on Hydrodynamic Viscosity and Selfgravitation in Accretion Disks
- ISOSCELES Project: II. Modelling galactic B-type stars for fast and delta- slow wind regimes
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