Photon bubbles in the circumstellar envelopes of young massive stars

Keyphrases

• Massive Stars 100%
• Bubble Instability 100%
• Circumstellar Envelopes 100%
• Shock 66%
• Gas Pressure 66%
• Optically Thick 33%
• Velocity Dispersion 33%
• Scale Height 33%
• Order of Magnitude 33%
• Dust Opacity 33%
• Growth Rate 33%
• Linear Analysis 33%
• Infrared Radiation 33%
• Magnetic Pressure 33%
• Magnetosonic 33%
• Pressure Scale 33%
• Eddington Limit 33%
• Low-density Material 33%
• High-mass Stars 33%
• Supersonic Motion 33%
• Maser Emission 33%

Physics

• Massive Star 100%
• Gas Pressure 100%
• Scale Height 50%
• Magnetohydrodynamic Generator 50%
• Supersonics 50%
• Infrared Radiation 50%
• Low Density Materials 50%
• High-Mass Stars 50%