ChangeGeometry(GRID[, center, rot_dict, …]) |
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DataTab_LIME(dens, temp, vel, abund, gtd, GRID) |
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DataTab_LIME2(dens_H2, dens_H, dens_Hp, …) |
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DataTab_RADMC3D_FreeFree(dens, temp, GRID) |
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MakeHole(T_min, T_max, dens_val, temp_val, …) |
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Make_Datatab1(prop_list, GRID[, …]) |
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PrintProperties(density, temperature, GRID) |
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Rotation_Matrix(angle_dicts) |
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abundance(val, NPoints) |
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abundance_Powerlaw(r_max, r_min, ab0, q, GRID) |
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abundance_PowerlawShells(r_list, p_list, …) |
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col_ids_LIME(props) |
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density_Constant(Rd, GRID[, discDens, …]) |
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density_Env_Disc(RStar, Rd, rhoE0, Arho, GRID) |
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density_Hamburgers(RStar, shFactor, Ro, …) |
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density_Hamburgers_piecewise(RStar, H0, …) |
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density_Keto_HII(MStar, r_min, r_max, rho_s, …) |
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density_Powerlaw(r_max, rho_mean, q, GRID[, …]) |
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density_Powerlaw2(r_max, r_min, rho0, q, GRID) |
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density_PowerlawShells(r_list, p_list, rho0, …) |
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density_Powerlaw_HII(r_min, r_max, r_s, …) |
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density_lyndenbell_disc(GRID[, Rc, Ec, …]) |
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gastodust(val, NPoints) |
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grid(XYZmax, NP[, rt_code, include_zero, …]) |
Computes the hosting grid for the model(s). |
sphe_cart(V_sphe, theta, phi) |
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streamline(Rd, GRID) |
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temperature(TStar, Rd, T10Env, RStar, MStar, …) |
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temperature_Constant(density, GRID[, …]) |
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temperature_Hamburgers(TStar, RStar, MStar, …) |
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temperature_Powerlaw(r_max, T_mean, q, GRID) |
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temperature_Powerlaw2(r_max, r_min, T0, q, GRID) |
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temperature_PowerlawShells(r_list, p_list, …) |
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velocity(RStar, MStar, Rd, density, GRID) |
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velocity_infall(dens_dict, ff_factor, MStar, …) |
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velocity_piecewise(density, GRID[, R_list, …]) |
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velocity_random(v_disp, NPoints) |
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