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High Excitation Gas and ISMAn 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 summarized, their diagnostic capabilities illustrated and their implications highlighted.
Document ID
20050010078
Acquisition Source
Ames Research Center
Document Type
Book
Authors
Peeters, E.
(NASA Ames Research Center Moffett Field, CA, United States)
Martin-Hernandez, N. L.
(Geneva Observatory Sauverny, Switzerland)
Rodriguez-Fernandez, N. J.
(Observatoire de Paris France)
Tielens, A. G. G. M.
(Kapteyn Astronomical Lab. Netherlands)
Date Acquired
August 22, 2013
Publication Date
June 10, 2004
Publication Information
Publication: ISO Mission Results: Space Science Reviews
Publisher: Kluwer Academic Publishers
Subject Category
Astrophysics
Funding Number(s)
CONTRACT_GRANT: HPMF-CT-2002-01677
Distribution Limits
Public
Copyright
Other

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