Dusty spirals triggered by shadows in transition discs

Keyphrases

• Thermal Emission 100%
• Radiative Transfer Calculation 100%
• Dust Particles 100%
• Transition Disks 100%
• Grain Growth 50%
• Near-infrared Spectrum 50%
• Physical Mechanism 50%
• Inner Region 50%
• Protoplanetary Disks 50%
• Hydrodynamic Simulation 50%
• Optically Thick 50%
• Planetesimals 50%
• Young Stars 50%
• Gravitational Perturbations 50%
• Fainting 50%
• Fixed Disc 50%
• Spiral Pattern 50%
• Well-mixed 50%
• Spiral Wave 50%
• Gaseous Phase 50%
• Perturbation Effect 50%
• Illumination Effect 50%
• Synthetic Observations 50%
• Dust Emission 50%
• Dynamical Effect 50%
• Dust Evolution 50%
• Active Discussions 50%
• Millimeter Wavelength 50%
• Shadow Cast 50%
• Spiral Shape 50%

INIS

• dusts 100%
• particles 75%
• emission 75%
• radiative transfer 50%
• dynamics 25%
• size 25%
• comparative evaluations 25%
• perturbations 25%
• distribution 25%
• simulation 25%
• grain growth 25%
• distance 25%
• trapping 25%
• wavelengths 25%
• torque 25%
• cavities 25%
• planets 25%
• protoplanets 25%
• illumination 25%

Physics

• Thermal Emission 100%
• Radiative Transfer 100%
• Near Infrared 50%
• Hydrodynamical Simulations 50%
• Protoplanets 50%
• Protoplanetary Disk 50%