High excitation ISM and gas
arXiv:astro-ph/0503711 · doi:10.1007/s11214-005-8070-1
Abstract
An overview is given of ISO results on regions of high excitation ISM and gas, i.e. HII regions, the Galactic Centre and Supernovae Remnants. IR emission due to fine-structure lines, molecular hydrogen, silicates, polycyclic aromatic hydrocarbons and dust are summarised, their diagnostic capabilities illustrated and their implications highlighted.
To be publised in the review book : "ISO science legacy - a compact review of ISO major achievements"