Radiative magneto-hydrodynamics in massive star formation and accretion disks
arXiv:1003.4861 · doi:10.1017/S174392130903018X
Abstract
We briefly overview our newly developed radiation transport module for MHD simulations and two actual applications. The method combines the advantage of the speed of the Flux-Limited Diffusion approximation and the high accuracy obtained in ray-tracing methods.
2 pages, 1 figure, Proceedings of the IAU Symposium 259, Cosmic Magnetic Fields: From Planets, to Stars and Galaxies