A radiation-driven disc wind model for massive young stellar objects

Keyphrases

• Young Stellar Objects 100%
• Wind Model 100%
• Disk Wind 100%
• Optically Thick 50%
• Escape Velocity 50%
• Irradiation 50%
• Rotator 50%
• Wind Speed 50%
• Keplerian Disc 50%
• Stellar Surfaces 50%
• Low Velocity 50%
• Mass Loss 50%
• Herbig 50%

Physics

• Young Stellar Objects 100%
• Stellar Surfaces 50%
• B Stars 50%
• Wind Velocity 50%