Radiative Transfer in 3-D Dusty Clouds and Circumstellar Disks

Introduction

I have built a new Monte Carlo radiative transfer code called RADMC-3D. It is the 3-D version of the RADMC code. Or better: it is a complete bottom-up rewrite of RADMC. It is written in Fortran 90 (as opposed to F77 for RADMC), it can treat 1-D, 2-D and 3-D geometries in cartesian or spherical coordinates, it has various options for gridding including grid refinement (AMR). And it has a Graphical User Interface for rendering images from a model, written in the IDL language. It has a number of example model setups, including one for a protoplanetary disk model (also with a GUI).

The home page of RADMC-3D has moved here.