# 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, except for the models with fragments. # Each row corresponds to a set of models. Columns are separated by the ampersand. # The first column lists model IDs in the set, second the model parameter that # was varied in that set, third the fiducial value of the parameter, fourth the # values that were explored in the set, fifth is the disc inclination of models # in the set (same in all models if a single value is given). Model IDs & Parameter & Fiducial & Values explored & Inclination (degrees) LIN_2 & Line choice & K = 3, J=13 -> 12 & K = 7, J=13 -> 12 & 30 INC_[N] & Inclination (degrees) & 30, 60 & N*10, N=0 to 9 & NSP_4 & Number of spirals & 2 & 4 & 30 NSP_0_INC_3,NSP_0_INC_6,NSP_0_INC_8 & Number of spirals & 2 & 0 & 30, 60, 80 ACC_1,ACC_2,ACC_3 & Accretion rate (Msun/yr) & 1e-3 & 1e-5, 1e-4, 1e-2 & 60 ETA_1,ETA_2 & Kinematic and thermal perturbation parameter & 0.2 & -0.2, 0.1 & 60 ANG_[N] & Rotational offset (rad) & 0 & N*pi/4, N=1 to 3 & 60 DIS_1,DIS_2 & Distance (kpc) & 3 & 1, 5 & 30 ATM_1,ATM_2,ATM_3 & Ratio of atmospheric to midplane temperature & 4 & 1, 2, 8 & 60 DUST_1,DUST_2 & Dust properties & a_max=1 cm, q=3.3 & a_max=0.1 um, q=3.3; a_max=1 cm, q=3.5 & 60