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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S270(6), p. 297-300, 2010

DOI: 10.1017/s1743921311000548

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Radiation-MHD Simulations of HII Region Expansion in Turbulent Molecular Clouds

Journal article published in 2010 by S. J. Arthur, W. J. Henney, G. Mellema ORCID, F. de Colle ORCID, E. Vázquez-Semadeni
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

AbstractWe use numerical simulations to investigate how the expansion of an HII region is affected by an ambient magnetic field. First we consider the test problem of expansion in a uniform medium with a unidirectional magnetic field. We then describe the expansion of an HII region in a turbulent medium, taking as our initial conditions the results of and MHD turbulence simulation. We find that although in the uniform medium case the magnetic field does produce interesting effects over long length and timescales, in the turbulent medium case the main effect of the magnetic field is to reduce the efficiency of fragmentation of the molecular gas.

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