Title of article :
NEI Modelling of the ISM – Turbulent Dissipation and Hausdorff Dimension
Author/Authors :
Miguel A. de Avillez، نويسنده , , Dieter Breitschwerdt، نويسنده ,
Issue Information :
روزنامه با شماره پیاپی سال 2009
Pages :
2
From page :
468
To page :
469
Abstract :
High-resolution non-ideal magnetohydrodynamical simulations of the turbulent magnetized ISM, powered by supernovae types Ia and II at Galactic rate, including self-gravity and non-equilibriuim ionization (NEI), taking into account the time evolution of the ionization structure of H, He, C, N, O, Ne, Mg, Si, S and Fe, were carried out. These runs cover a wide range (from kpc to sub-parsec) of scales, providing resolution independent information on the injection scale, extended self-similarity and the fractal dmension of the most dissipative structures.
Journal title :
Proceedings of the International Astronomical Union
Serial Year :
2009
Journal title :
Proceedings of the International Astronomical Union
Record number :
674776
Link To Document :
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