NEI Modelling of the ISM - Turbulent Dissipation & Hausdorff Dimension

Details NEI Modelling of the ISM - Turbulent Dissipation & Hausdorff Dimension NEI Modelling of the ISM - Turbulent Dissipation & Hausdorff Dimension

2009-10-12

arxiv.org/abs/0910.2216v1

Astronomy and Astrophysics

Astrophysics

Galaxy Astrophysics

2 pages, 1 figure. Invited talk to the Joint Discussion 15 "Magnetic Fields in Diffuse Media". To appear in Highlights of Astr

Scientific paper

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.

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