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Radiative magneto-hydrodynamics in massive star formation and accretion disks

Published online by Cambridge University Press:  01 November 2008

Rolf Kuiper ,
Mario Flock  and
Hubert Klahr
Rolf Kuiper
Affiliation:
Max-Planck Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany email: [email protected]
Mario Flock
Affiliation:
Max-Planck Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany email: [email protected]
Hubert Klahr
Affiliation:
Max-Planck Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany email: [email protected]
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Abstract

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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.

Keywords

Radiative transfer – MHD – stars: formation – accretion disks – methods: numerical
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 4 , Symposium S259: Cosmic Magnetic Fields: From Planets, to Stars and Galaxies , November 2008 , pp. 103 - 104
Copyright
Copyright © International Astronomical Union 2009

References

Levermore, C. D. & Pomraning, G. C. 1981, ApJ 248, 321CrossRefGoogle 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, 23CrossRefGoogle Scholar