Please use this identifier to cite or link to this item:
http://hdl.handle.net/10174/5641
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| Title: | NEI Modelling of the ISM - Turbulent Dissipation and Hausdorff Dimension |
| Authors: | de Avillez, Miguel
Breitschwerdt, Dieter |
| Editors: | Corbett, Ian
et al. |
| Issue Date: | Nov-2010 |
| Publisher: | Cambridge University Press/International Astronomical Union |
| 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. |
| URI: | http://hdl.handle.net/10174/5641 |
| Type: | article |
| Appears in Collections: | MAT - Artigos em Livros de Actas/Proceedings
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