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
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
years
2026 2verdicts
UNVERDICTED 2representative citing papers
Radiative cooling thins hot accretion disks around black holes, reduces wind power, and makes inflow-rate decrease depend more on MRI-driven turbulence than on winds as cooling strengthens.
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.
-
Radiative cooling effects on black hole hot accretion flows around the sub-Bondi radius
Radiative cooling thins hot accretion disks around black holes, reduces wind power, and makes inflow-rate decrease depend more on MRI-driven turbulence than on winds as cooling strengthens.