The DIRTY Model. I. Monte Carlo Radiative Transfer through Dust

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© 2001. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Karl D. Gordon et al 2001 ApJ 551 269 DOI 10.1086/320082

0004-637X/551/1/269

Abstract

We present the DIRTY (DustI Radiative Transfer, Yeah!) radiative transfer model in this paper and a companion paper. This model computes the polarized radiative transfer of photons from arbitrary distributions of stars through arbitrary distributions of dust using Monte Carlo techniques. The dust re-emission is done self-consistently with the dust absorption and scattering and includes all three important emission paths: equilibrium thermal emission, nonequilibrium thermal emission, and the aromatic features emission. The algorithm used for the radiative transfer allows for the efficient computation of the appearance of a model system as seen from any viewing direction. We present a simple method for computing an upper limit on the output quantity uncertainties for Monte Carlo radiative transfer models that use the weighted photon approach.

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10.1086/320082