Herschel and Galaxies/AGN
| dc.creator | Barthel, Peter | |
| dc.date | 2004-11-24 | |
| dc.date.accessioned | 2026-07-07T02:16:00Z | |
| dc.date.available | 2026-07-07T02:16:00Z | |
| dc.description | Herschel will represent a breakthrough in the study of nearby gas-rich and gas-poor galaxies, as it will for the first time permit imaging photometric and spectroscopic observations of their ISM in the FIR-submm wavelength range. The unprecedented sensitivity and angular resolution of Herschel will furthermore yield a breakthrough in our understanding of distant galaxies and AGN, as their gas and dust - both the ISM- and the AGN-related - will for the first time come within reach. Herschel will undoubtedly yield major discoveries concerning the cosmologically evolving gas and dust properties in galaxies, back to very early epochs. | |
| dc.description | Invited review, at conference "The Dusty and Molecular Universe - A Prelude to HERSCHEL and ALMA", Paris, 27-29 October 2004 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0411659 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0411659 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/8624 | |
| dc.subject | Astrophysics | |
| dc.title | Herschel and Galaxies/AGN | |
| dc.type | text |