New Hydrodynamic Solutions for Line-driven Winds of Hot Massive Stars Using the Lambert W-function
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/ac12c9/pdf
Reference65 articles.
1. The theory of radiatively driven stellar winds. II - The line acceleration
2. ANALYTICAL SOLUTIONS FOR RADIATION-DRIVEN WINDS IN MASSIVE STARS. I. THE FAST REGIME
3. The Chemical Composition of the Sun
4. New predictions for radiation-driven, steady-state mass-loss and wind-momentum from hot, massive stars
5. Properties of Galactic early-type O-supergiants
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