High excitation ISM and gas

Details High excitation ISM and gas High excitation ISM and gas

2005-03-31

arxiv.org/abs/astro-ph/0503711v1

Space Science Reviews 2005

Astronomy and Astrophysics

Astrophysics

To be publised in the review book : "ISO science legacy - a compact review of ISO major achievements"

Scientific paper

10.1007/s11214-005-8070-1

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.

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