High Excitation ISM and Gas
2005
An overview is given of ISO results on regions of high excitation ISM and gas, i.e. HII regions, the Galactic Centre and Supernova 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.
Keywords:
- Correction
- Source
- Cite
- Save
- Machine Reading By IdeaReader
145
References
5
Citations
NaN
KQI