2005/06/17 by S. Wolf, Lynne A. Hillenbrand, L. A. Hillenbrand
Physics and Astronomy · #Astro and Planetary Science #Astrophysics #Astrophysics and Star Formation Studies #Atmospheric radiative transfer codes #Byte #Computational science #Computer hardware #Computer science #Debris disk #Fortran #Operating system #Optics #Perl #Physics #Radiative transfer #Spectral energy distribution #Spectral line #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1016/j.cpc.2005.04.014
published as Comput.Phys.Commun. 171 (2005) 208-218 · Comp. Phys. Comm, 2005, in press
arxiv created 2005/06/17 · openalex publication_date 2005/06/20 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
A WWW interface for the simulation of spectral energy distributions of optically thin dust configurations with an embedded radiative source is presented. The density distribution, radiative source, and dust parameters can be selected either from an internal database or defined by the user. This tool is optimized for studying circumstellar debris disks where large grains are expected to determine the far-infrared through millimeter dust reemission spectral energy distribution. The tool is available at http://aida28.mpia-hd.mpg.de/~swolf/dds