Back to Search Start Over

High excitation ISM and gas

Source :
Space science reviews. 119(1-4):273-292
Publication Year :
2005

Abstract

An overview is given of ISO results on regions of high excitation ISM and gas, i.e. H II 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.

Details

Language :
English
ISSN :
00386308
Volume :
119
Issue :
1-4
Database :
OpenAIRE
Journal :
Space science reviews
Accession number :
edsair.dris...01423..ff4f34931e9a3800df98db60f72a9a39