Debris Disk Radiative Transfer Simulation Tool (DDS)

Abstract

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

Comp. Phys. Comm, 2005, in press

References in corpus (4)

• A dust ring around Epsilon Eridani: analogue to the young Solar System
• Mie Scattering by Ensembles of Particles with Very Large Size Parameters
• MC3D - 3D Continuum Radiative Transfer, Version 2
• The Formation and Evolution of Planetary Systems: SIRTF Legacy Science in the VLT Era

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• Epsilon Eridani's Planetary Debris Disk: Structure and Dynamics based on Spitzer and CSO Observations
• Azimuthal asymmetries in the debris disk around HD61005
• Transient dust in warm debris disks - Detection of Fe-rich olivine grains
• Multi-wavelength modeling of the spatially resolved debris disk of HD 107146
• A peculiar class of debris disks from Herschel/DUNES - A steep fall off in the far infrared
• Extinction and the Dimming of KIC 8462852
• Dust production in the debris disk around HR 4796 A
• Extreme Variability of the V488 Persei Debris Disk
• High contrast optical imaging of companions: the case of the brown dwarf binary HD-130948BC
• Herschel Observations and Updated Spectral Energy Distributions of Five Sunlike Stars with Debris Disks
• Hiding Dust Around $\epsilon$ Eridani
• Dust Production Rates in the Fomalhaut Debris Disk from SOFIA/FORCAST Mid-infrared Imaging
• Review and prospects of hot exozodiacal dust research for future exo-Earth direct imaging missions
• Isolating the extreme debris disc signature -- explorations of eccentric extreme debris discs formed by giant impacts