Published in
Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S259(4), p. 103-104, 2008
DOI: 10.1017/s174392130903018x
Links
Tools
Radiative magneto-hydrodynamics in massive star formation and accretion disks
This paper was not found in any repository, but could be made available legally by the author.
Full text: Unavailable
Published version:
archiving forbidden
Data provided by 
Abstract
AbstractWe 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.
