# Observing substructure in circumstellar discs around massive young stellar objects # M. R. Jankovic, T. J. Haworth, J. D. Ilee, D. H. Forgan, C. J. Cyganowski, C. # Walsh, C. L. Brogan, T. R. Hunter, and S. Mohanty, 2018, accepted in MNRAS # Summary of models with spiral arms and with fragments. # Disc inclination is 30 degrees. The rest of the disc model parameters are fiducial # values in the file models_table_spiral.dat # First column is model ID, second is orbital distance of the fragment (clump) in the # disc, third is fragment mass and fourth is fragment temperature. Model ID & Orbital distance (AU) & Mass (Msol) & Temperature (K) CLUMP_1 & 800 & 5 & 1400 CLUMP_2 & 200 & 5 & 1400 CLUMP_3 & 800 & 2 & 150 CLUMP_4 & 800 & 0.1 & 150 CLUMP_5 & 800 & 0.1 & 300 CLUMP_6 & 800 & 0.1 & 700 CLUMP_7 & 800 & 0.1 & 1400 CLUMP_8 & 800 & 5 & 700