Diskenv is a Python framework to compute the continuum and line emission of young stellar objects (protostars, disks. etc.). It is based on RADMC-3D.
It was originally developed to model disks in embedded protostars (hence its name), but it has evolved into a more general purpose framework. It now allows to build models of astronomical sources from user-provided density and velocity values (for example from an analytical prescription), or from a numerical simulation (currently only the Idefix format is supported).
Diskenv requires radmc3d. Make sure the executable in the PATH
environnement variable. In addition, Idefix's pytools module must be
in the PYTHONPATH for the Idefix data import to work.
Diskenv and its dependencies can be installed with:
pip install .
See the example/ directory for some examples of use.