Hostname: page-component-7c8c6479df-24hb2 Total loading time: 0 Render date: 2024-03-27T05:42:42.413Z Has data issue: false hasContentIssue false

Radiative magneto-hydrodynamics in massive star formation and accretion disks

Published online by Cambridge University Press:  01 November 2008

Rolf Kuiper
Affiliation:
Max-Planck Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany email: kuiper@mpia.de
Mario Flock
Affiliation:
Max-Planck Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany email: kuiper@mpia.de
Hubert Klahr
Affiliation:
Max-Planck Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany email: kuiper@mpia.de
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2009

References

Levermore, C. D. & Pomraning, G. C. 1981, ApJ 248, 321Google Scholar
Fromang, S. & Nelson, A. P. 2006, A&A 457, 343Google Scholar
Mignone, A., Bodo, G., Massaglia, S.Matsakos, T., Tesileanu, O., Zanni, C., & Ferrari, A. 2007, ApJ 170, 228Google Scholar
Pascucci, I., Wolf, S., Steinacker, J., et al. 2004, A&A 417, 793Google Scholar
Shu, F. H., Adams, F. C., & Lizano, S. 1987, ARAA 25, 23Google Scholar