A Non-Equilibrium Ionization Model of the Local and Loop I Bubbles - Tracing the Ovi Distribution

Details A Non-Equilibrium Ionization Model of the Local and Loop I Bubbles - Tracing the Ovi Distribution A Non-Equilibrium Ionization Model of the Local and Loop I Bubbles - Tracing the Ovi Distribution

2011-08-31

arxiv.org/abs/1108.6226v1

Astronomy and Astrophysics

Astrophysics

Galaxy Astrophysics

To be published in "Advances in Computational Astrophysics: Methods, Tools and Outcomes", R. Dolcetta, M. Limongi, A. Tornambe

Scientific paper

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.

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