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MC3D: Monte-Carlo 3D Radiative Transfer Code

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MC3D: Monte-Carlo 3D Radiative Transfer Code

Postby owlice » Tue Apr 03, 2012 8:20 pm

MC3D: Monte-Carlo 3D Radiative Transfer Code

Abstract: MC3D is a 3D continuum radiative transfer code; it is based on the Monte-Carlo method and solves the radiative transfer problem self-consistently. It is designed for the simulation of dust temperatures in arbitrary geometric configurations and the resulting observables: spectral energy distributions, wavelength-dependent images, and polarization maps. The main objective is the investigation of "dust-dominated" astrophysical systems such as young stellar objects surrounded by an optically thick circumstellar disk and an optically thin(ner) envelope, debris disks around more evolved stars, asymptotic giant branch stars, the dust component of the interstellar medium, and active galactic nuclei.

Credit: Wolf, S.; Henning, T.; Stecklum, B.

Site: http://portia.astrophysik.uni-kiel.de/~ ... seite=mc3d
http://adsabs.harvard.edu/abs/1999A%26A...349..839W

Bibcode: 2012ascl.soft04005W

ID: ascl:1204.005
Last edited by Ada Coda on Sun Dec 30, 2018 7:51 pm, edited 1 time in total.
Reason: Updated code entry.
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