=========================== Output from program Dusty Version: 2.0 =========================== INPUT parameters from file: sphere1.inp * ---------------------------------------------------------------------- * NOTES: * This is a simple version of an input file producing a minimal output. * ---------------------------------------------------------------------- Central source spectrum described by a black body with temperature: 2500 K -------------------------------------------- Abundances for supported grains: Sil-Ow Sil-Oc Sil-DL grf-DL amC-Hn SiC-Pg 1.000 0.000 0.000 0.000 0.000 0.000 MRN size distribution: Power q: 3.5 Minimal size: 5.00E-03 microns Maximal size: 2.50E-01 microns -------------------------------------------- Dust temperature on the inner boundary: 800 K -------------------------------------------- Density described by 1/r**k with k = 2.0 Relative thickness: 1.000E+03 -------------------------------------------- Optical depth at 5.5E-01 microns: 1.00E+00 Required accuracy: 5% -------------------------------------------- ==================================================== For compliance with the point-source assumption, the following results should only be applied to sources whose effective temperature exceeds 1737 K. ==================================================== RESULTS: -------- ### tau0 F1(W/m2) r1(cm) r1/rc theta1 Td(Y) err ### 1 2 3 4 5 6 7 ========================================================== 1 1.00E+00 2.88E+04 3.26E+14 8.78E+00 2.43E+00 44 0 ========================================================== (1) Optical depth at 5.5E-01 microns (2) Bolometric flux at the inner radius (3) Inner radius for L=1E4 Lsun (4) Ratio of the inner to the stellar radius (5) Angular size (in arcsec) when Fbol=1E-6 W/m2 (6) Dust temperature at the outer edge (in K) (7) Maximum error in flux conservation (%) ================================================= Everything is OK for all models ========== THE END ==============================