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Article Dans Une Revue Space Science Reviews Année : 2005

High Excitation ISM and Gas

Résumé

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.

Dates et versions

hal-03797004 , version 1 (04-10-2022)

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Citer

Els Peeters, Nieves Leticia Martín-Hernández, N. J. Rodriguez-Fernandez, Xander Tielens. High Excitation ISM and Gas. Space Science Reviews, 2005, 119, pp.273-292. ⟨10.1007/s11214-005-8070-1⟩. ⟨hal-03797004⟩
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