Evolution of rotating massive stars with new hydrodynamic wind models

Keyphrases

• Massive Stars 100%
• Wind Model 100%
• Mass Loss 50%
• Mass Loss Rate 50%
• Weak Winds 50%
• Evolutionary 33%
• Metallicity 33%
• Galactic 33%
• Stellar Rotation 33%
• Evolution Model 33%
• Main Sequence 33%
• Evolutionary Model 16%
• Low-mass 16%
• Research-based 16%
• Angular Momentum 16%
• Correction Factor 16%
• High Brightness 16%
• K Parameter 16%
• Galactic Center 16%
• Stellar Winds 16%
• Stellar Evolution 16%
• Interstellar Medium 16%
• Helium 16%
• Self-consistent Model 16%
• Rotational Velocity 16%
• Force Parameters 16%
• Force Line 16%
• O-type 16%
• Additional Term 16%
• Multiple Systems 16%
• Single System 16%
• 26Al 16%
• Massive Models 16%
• Self-consistent Approach 16%
• Large Magellanic Cloud 16%
• Mixing Efficiency 16%
• Simultaneous Calculations 16%
• Stellar Structure 16%

INIS

• wind 100%
• hydrodynamics 100%
• mass loss 85%
• tracks 57%
• rotation 57%
• range 28%
• values 28%
• grids 28%
• metallicity 28%
• abundance 14%
• surveys 14%
• populations 14%
• surfaces 14%
• solutions 14%
• acceleration 14%
• mixing 14%
• corrections 14%
• reduction 14%
• stars 14%
• velocity 14%
• luminosity 14%
• angular momentum 14%
• stellar winds 14%
• star evolution 14%
• helium 14%
• isotopes 14%
• aluminium 26 14%
• magellanic clouds 14%

Physics

• Massive Star 100%
• Metallicity 33%
• Stellar Rotation 33%
• Angular Momentum 16%
• Galactic Center 16%
• Stellar Wind 16%
• Interstellar Matter 16%
• Stellar Structure 16%
• Large Magellanic Cloud 16%
• Stellar Evolution 16%