1204.1511 (M. A. de Avillez et al.)

Electron Distribution in the Galactic Disk - Results From a Non-Equilibrium Ionization Model of the ISM    [PDF]

M. A. de Avillez, A. Asgekar, D. Breitschwerdt, E. Spitoni

Using three-dimensional non-equilibrium ionization (NEI) hydrodynamical simulation of the interstellar medium (ISM), we study the electron density, $n_{e}$, in the Galactic disk and compare it with the values derived from dispersion measures towards pulsars with known distances located up to 200 pc on either side of the Galactic midplane. The simulation results, consistent with observations, can be summarized as follows: (i) the DMs in the simulated disk lie between the maximum and minimum observed values, (ii) the log derived from lines of sight crossing the simulated disk follows a Gaussian distribution centered at \mu=-1.4 with a dispersion \sigma=0.21, thus, the Galactic midplane =0.04\pm 0.01$ cm$^{-3}$, (iii) the highest electron concentration by mass (up to 80%) is in the thermally unstable regime (200View original: http://arxiv.org/abs/1204.1511