A Non-Equilibrium Ionization Model of the Local and Loop I Bubbles - Tracing the Ovi Distribution
Astrophysics of Galaxies
2011-09-01 v1 High Energy Astrophysical Phenomena
Abstract
We present the first to date three-dimensional high-resolution hydrodynamical simulation tracing the non-equilibrium ionization evolution (using the Eborae Atomic and Molecular Plasma Emission Code - E(A+M)PEC) of the Local Bubble and Loop I superbubbles embedded in a turbulent supernova-driven interstellar medium.
Keywords
Cite
@article{arxiv.1108.6226,
title = {A Non-Equilibrium Ionization Model of the Local and Loop I Bubbles - Tracing the Ovi Distribution},
author = {Miguel A. de Avillez and Dieter Breitschwerdt and Emanuele Spitoni and Nuno Carvalho},
journal= {arXiv preprint arXiv:1108.6226},
year = {2011}
}
Comments
To be published in "Advances in Computational Astrophysics: Methods, Tools and Outcomes", R. Dolcetta, M. Limongi, A. Tornambe (Editors), ASP Conf. Series