NEI Modelling of the ISM - Turbulent Dissipation and Hausdorff Dimension
| dc.contributor.author | de Avillez, Miguel | |
| dc.contributor.author | Breitschwerdt, Dieter | |
| dc.contributor.editor | Corbett, Ian | |
| dc.contributor.editor | et al. | |
| dc.date.accessioned | 2012-11-15T14:22:01Z | |
| dc.date.available | 2012-11-15T14:22:01Z | |
| dc.date.issued | 2010-11 | |
| dc.description.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. | por |
| dc.identifier.authoremail | mavillez@galaxy.lca.uevora.pt | |
| dc.identifier.authoremail | breitschwerdt@astro.physik.tu-berlin.de | |
| dc.identifier.doi | 10.1017/S1743921310010318 | |
| dc.identifier.pagina | 468-469 | |
| dc.identifier.principalpublicationtitle | Highlights of Astronomy | |
| dc.identifier.scientificarea | 343 | por |
| dc.identifier.uri | http://hdl.handle.net/10174/5641 | |
| dc.identifier.volume | 15 | |
| dc.language.iso | eng | por |
| dc.peerreviewed | yes | por |
| dc.publisher | Cambridge University Press/International Astronomical Union | por |
| dc.rights | openAccess | por |
| dc.title | NEI Modelling of the ISM - Turbulent Dissipation and Hausdorff Dimension | por |
| dc.type | article | por |