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