Continuum and line modelling of discs around young stars - I. 300 000 disc models for HERSCHEL/GASPS

Engineering

• Distribution Line 100%
• Energy Distribution 100%
• Chemical Structure 100%
• Observables 100%
• Shape Parameter 100%
• Detection Limit 100%
• Input Parameter 100%

Physics

• Radiative Transfer 100%
• Circumstellar Disks 100%
• Fine Structure 50%
• Spectral Energy Distribution 50%
• Monte Carlo 50%
• Disks (Shapes) 50%
• Disk Flaring 50%
• Data Interpretation 50%
• Gas-to-Dust Ratio 50%
• Stellar Disks 50%

Earth and Planetary Sciences

• Radiative Transfer 100%
• Data Interpretation 50%
• Fine Structure 50%
• Flaring 50%
• Chemical Structure 50%
• Thermochemical 50%
• Disks (Shapes) 50%
• Spectral Energy Distribution 50%