H i in Molecular Clouds: Irradiation by FUV Plus Cosmic Rays

Keyphrases

• Cosmic Rays 100%
• Irradiation 100%
• Molecular Clouds 100%
• Far Ultraviolet 100%
• Giant Molecular Clouds 83%
• Cosmic Ray Ionization 66%
• Column Density 50%
• Ionization Rate 50%
• Ultraviolet Photodissociation 50%
• Galactic 33%
• Dust 33%
• Attenuation 16%
• Steady State 16%
• Density Profile 16%
• Transport Effects 16%
• Field Strength 16%
• Gas Density 16%
• Analytic Expression 16%
• Atomic Hydrogen 16%
• Formation Rate 16%
• Rate Coefficients 16%
• H2 Formation 16%
• Analytic Theory 16%
• Hydrogen Gas 16%
• Depth-dependent 16%
• Dust-to-gas Ratio 16%
• Cosmic Ray Flux 16%
• Self-shielding 16%
• Low Energy Cosmic Rays 16%

Physics

• Molecular Clouds 100%
• Giant Molecular Clouds 100%
• Photodissociation 60%
• M Giant Stars 40%
• Steady State 20%
• Field Strength 20%
• Transition Point 20%
• Gas-to-Dust Ratio 20%

Earth and Planetary Sciences

• Molecular Clouds 100%
• Photodissociation 50%
• Transition Point 16%
• Field Strength 16%
• Gas Density 16%