The documentation of astroMUGS

A modular and user-friendly pipeline to couple MHD, radiative transfer, and chemistry, for MUlti-Grain Simulations (MUGS), specifically dedicated to young stellar objects. astroMUGS is the new version of the library chemdiskpy.

User Guide

This is where it all begins.

• Quickstart
  • Introduction
  • Installation of astroMUGS
  • How to use the code
• astroMUGS in details
  • The Grid
  • The Disk model
  • The Model class
  • Input files
  • Radiative transfer simulations
  • Gas-grain simulations
  • RADMC3D – Nautilus coupling
  • API Reference
• Graphical User Interface: astroMUGS-ui
  • Introduction
  • Installation
  • Run astroMUGS-ui