Rolf Kuiper, Mario Flock, Hubert Klahr
Published 2010-03-25Version 1
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.
Comments: 2 pages, 1 figure, Proceedings of the IAU Symposium 259, Cosmic Magnetic Fields: From Planets, to Stars and Galaxies
Journal: Cosmic Magnetic Fields: From Planets, to Stars and Galaxies, Proceedings of the International Astronomical Union, IAU Symposium, Volume 259, p. 103-104 (2009)
The Herschel view of massive star formation in G035.39--00.33: Dense and cold filament of W48 undergoing a mini-starburst
The VLT-FLAMES Tarantula Survey. XXIX. Massive star formation in the local 30 Doradus starburst
Accretion disks around massive stars: Hydrodynamic structure, stability and dust sublimation
![QR code for arXiv:1003.4861 [astro-ph.SR]](http://oss.arxitics.com/images/favicon.svg)