The project will use the adaptive mesh radiative magnetohydrodynamic simulation code RAMSES to model the evolution of nebulae in the Large and Small Magellanic Clouds neighbouring our Milky Way galaxy. The project will use the results of the previous 500 khr Cartesius project AMUN, which focussed on Orion and other Milky Way clouds, to explore wider conditions in the universe. This is timely because our group in Amsterdam is heavily involved in the VFTS survey of the LMC which requires theoretical interpretation, while collaborating groups in Leiden and Heidelberg are active in the new and upcoming surveys SOFIA and SDSS-V targetting this galaxy. The project is split into three subprojects: a large pathfinder for a full simulation of the 30 Doradus region, a zoom-in project supporting the successful HPC Europa 3 grant by Raphael Mignon-Risse to visit UvA and SURF, and a project exploring the dynamics and environment of large cloud complexes using targetted simulations. The project is integral to my research at API and to the science questions of the group at API/UvA and wider NOVA-network institutions.