| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1780077 | New Astronomy Reviews | 2009 | 5 Pages |
Abstract
The FIR/submm window is amongst the least explored spectral regions of the electromagnetic spectrum. It is, however, a key to study the general properties of the interstellar medium of galaxies, as it contains important spectral line diagnostics from the neutral, ionized and molecular ISM. The Herschel Space Observatory, successfully launched on 14 May 2009, is the first observatory to cover the entire FIR/submm range between 57 and 672 μm. We discuss the main results from the ISO era on FIR spectroscopy of galaxies and the enormous science potential of the Herschel mission through a presentation of its spectroscopic extragalactic key programs.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
Maarten Baes, Suzanne C. Madden, Christine D. Wilson, Andreas A. Lundgren, Carlos De Breuck,