3.0 mcfost version #Number of photon packages 1.28e8 nbr_photons_eq_th : T computation 1.28e3 nbr_photons_lambda : SED computation 1.28e8 nbr_photons_image : images computation #Wavelength 50 0.1 3000.0 n_lambda, lambda_min, lambda_max [mum] Do not change this line unless you know what you are doing T F T compute temperature?, compute sed?, use default wavelength grid for output ? IMLup.lambda wavelength file (if previous parameter is F) T T separation of different contributions?, stokes parameters? #Grid geometry and size 1 1 = cylindrical, 2 = spherical (a Voronoi mesh is selected automatically with -phantom) 100 70 1 20 n_rad (log distribution), nz (or n_theta), n_az, n_rad_in #Maps 1000 1000 400. grid (nx,ny), size [AU] 0. 90. 1 F RT: imin, imax, n_incl, centered ? 0 0. 1 RT: az_min, az_max, n_az angles 104.2 distance (pc) 0. disk PA #Scattering method 0 0=auto, 1=grain prop, 2=cell prop 1 1=exact phase function, 2=hg function with same g (2 implies the loss of polarizarion) #Symetries F image symmetry F central symmetry F axial symmetry (important only if N_phi > 1) #Disk physics 0 0.50 1.0 dust_settling (0=no settling, 1=parametric, 2=Dubrulle, 3=Fromang), exp_strat, a_strat (for parametric settling) F dust radial migration F sublimate dust F hydostatic equilibrium F 1e-5 viscous heating, alpha_viscosity #Number of zones : 1 zone = 1 density structure + corresponding grain properties 1 needs to be 1 if you read a density file (phantom or fits file) #Density structure 1 zone type : 1 = disk, 2 = tappered-edge disk, 3 = envelope, 4 = debris disk, 5 = wall 1.e-3 45. dust mass, gas-to-dust mass ratio 10. 100.0 2 scale height, reference radius (AU), unused for envelope, vertical profile exponent (only for debris disk) 1.0 0.0 300. 100. Rin, edge, Rout, Rc (AU) Rc is only used for tappered-edge & debris disks (Rout set to 8*Rc if Rout==0) 1.125 flaring exponent, unused for envelope -0.5 0.0 surface density exponent (or -gamma for tappered-edge disk or volume density for envelope), usually < 0, -gamma_exp (or alpha_in & alpha_out for debris disk) #Grain properties 1 Number of species Mie 1 2 0.0 1.0 0.9 Grain type (Mie or DHS), N_components, mixing rule (1 = EMT or 2 = coating), porosity, mass fraction, Vmax (for DHS) Draine_Si_sUV.dat 1.0 Optical indices file, volume fraction 1 Heating method : 1 = RE + LTE, 2 = RE + NLTE, 3 = NRE 0.03 1000.0 3.5 100 amin, amax [mum], aexp, n_grains (log distribution) #Molecular RT settings T T T 15. lpop, laccurate_pop, LTE, profile width [km/s] 0.05 Turbulence velocity [km/s] 1 Number of molecules co.dat 6 molecular data filename, level max up to which NLTE populations are calculated 6.345 150 vmax [km/s], number of velocity bins betwen 0 and vmax T 1.e-4 abundance.fits.gz cst molecule abundance ?, abundance, abundance file T 2 ray tracing ?, number of lines in ray-tracing 2 3 transition numbers #Star properties 3 Number of stars 7250.0 1.58 1.7 0.0 0.0 0.0 T Temp, radius (solar radius),M (solar mass),x,y,z (AU), is a blackbody? lte7200-3.5.NextGen.fits.gz 0.0 2.2 fUV, slope_fUV 3250.0 0.75 0.2 0.0 0.0 0.0 T Temp, radius (solar radius),M (solar mass),x,y,z (AU), is a blackbody? lte3300-3.5.NextGen.fits.gz 0.0 2.2 fUV, slope_fUV 3250.0 0.001 0.00001 0.0 0.0 0.0 T Temp, radius (solar radius),M (solar mass),x,y,z (AU), is a blackbody? lte3300-3.5.NextGen.fits.gz 0.0 2.2 fUV, slope_fUV Executed command line : mcfost HD100453.para -phantom mydisc -mol -fix_star -freeze-out 20 -photo-dissociation -photo-desorption -mol Fri 29 May 09:35:34 BST 2020 Linux dirac04 3.10.0-1062.18.1.el7.x86_64 #1 SMP Tue Mar 17 23:49:17 UTC 2020 x86_64 x86_64 x86_64 GNU/Linux sha = 5470200caa115a1adb6045520c96f3d129536cb2