Super-Eddington stellar winds: Unifying radiative-enthalpy versus flux-driven models

Keyphrases

• Eddington 100%
• Driving Model 100%
• Stellar Winds 100%
• Flux Control 100%
• Luminosity 80%
• Optically Thick 40%
• Massive Stars 40%
• Radiative Fluxes 40%
• Energy Addition 20%
• Escape Velocity 20%
• Eddington Luminosity 20%
• Advection 20%
• Wind Speed 20%
• Large Values 20%
• Radiative Diffusion 20%
• Asymptotic Limit 20%
• Gravitational Potential 20%
• Wind Model 20%
• Steady Solution 20%
• Mass Loss 20%
• Semi-analytical Solution 20%
• Wind-induced 20%
• Mass Loss Rate 20%
• Stellar Mergers 20%
• Surface Heating 20%
• Coupled Differential Equations 20%
• Steady Wind 20%
• Classical Novae 20%
• Limit Models 20%
• Heating Radius 20%

Physics

• Enthalpy 100%
• Massive Star 100%
• Stellar Wind 100%
• Advection 50%
• Gravitational Field 50%
• Operators (Mathematics) 50%
• Wind Velocity 50%
• Classical Novae 50%