#Input parameters for sYSOm model #******************************** # --------------------------------- # Circumstellar dust-disc parameters # --------------------------------- Rin = 1.0 # Disc inner radius (AU). Rout = 10.0 # Disc outer radius (AU). 2*Rd is the image size in each direction dust_kappa_format = kappa_am_olivine_0.1_3000 #Dust opacity (kappa) model #T_disc_param # T_format = POWER_LAW # Type of dust-disc temperature law Tin = 1000.0 # Temperature at the basis of the dust-disc (K) powT = -0.5 # Dust-disc temperature power-law coefficient (param q) #dens_disc_params # density_format = SURF_DENS_POWER_LAW # Type of dust-disc density law powdens = -1.5 # Dust-disc density power-law coefficient (param p) density_input_key = MASS # Type of input key for density calculations (Mass or Sigma_in) density_param = 1.0e-7 # Density parameter: disc mass (Msun) or surface density at Rin (kg/m^2) # ------------------------------------ # Geometrical and numerical parameters # ------------------------------------ inclination = 60.0 # Inclination angle of star+disc (deg) distance = 100.0 # Distance to the star (pc) Npix = 256 # Nb of image pixels in each direction (x and y) # ----------------------- # Central star parameters # ----------------------- add_central_star = True # Flag indicating if a central star is to be added to the model # If the flag add_central_star is True then provide the central star parameters # Spherical star model (blackbody) Rstar = 2.0 # Stellar radius (Rsun) Tstar = 5000.0 # Effective temperature of the central star (K) compute_flux = True # Flag indicating if the flux (SED) will be computed compute_fits = True # Get the image in fits format # ----------------- # Spectral coverage # ----------------- wlen0 = 1.0 # Start wavelength (microns) dwlen = 1.0 # Wavelength step (microns) Nwlen = 12 # Nb of wavelength points