New stable wind solutions fill the elusive gap between fast and δ-slow radiation-driven regimes, showing velocity kinks and distinct H I, He I, Si IV line profiles.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.SR 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
Radiation-driven stellar winds at the fast-slow transition: new hydrodynamic solutions
New stable wind solutions fill the elusive gap between fast and δ-slow radiation-driven regimes, showing velocity kinks and distinct H I, He I, Si IV line profiles.