A Mid-Infrared and Far-Infrared View of Galaxies
arXiv:astro-ph/9909369 · doi:10.1023/A:1017084627953
Abstract
From the disk of normal galaxies to the nucleus of prototype active sources, we review the wealth of results and new understanding provided by recent infrared probes and, in particular, the four instruments on-board of ISO.
Review presented at the Millenium Conference on Galaxy Morphology (D. Block, I. Puerari, A. Stockton, dW. Ferreira Eds), Johannesburg, South Africa. 18 pages, 4 figures (fig3 is provided in gif to cut on size, should be converted to postscript). Includes the kluwer style files
References in corpus (10)
- Star Formation in Galaxies Along the Hubble Sequence
- What Powers Ultra-luminous IRAS Galaxies?
- The nature and evolution of Ultraluminous Infrared Galaxies: A mid-infrared spectroscopic survey
- ISO LWS Spectroscopy of M82: A Unified Evolutionary Model
- High Spatial Resolution Imaging of Arp 220 from 3 - 25 microns
- Molecular Gas Depletion and Starbursts in Luminous Infrared Galaxy Mergers
- Properties of Hot Stars in the Wolf-Rayet galaxy NGC5253 from ISO Spectroscopy
- SCUBA imaging of NGC 7331 dust ring
- Mid-Infrared Images of Luminous Infrared Galaxies in a Merging Sequence
- ISOCAM Mid-Infrared Imaging of the Quiescent Spiral Galaxy NGC 7331
Cited by in corpus (7)
- Warm dust and aromatic bands as quantitative probes of star-formation activity
- Mid-IR Observations of Mass Loss in Elliptical Galaxies
- ISOCAM view of the starburst galaxies M82, NGC253, and NGC1808
- Mid-Infrared Spectral Measures of Star-Formation and AGN Activity in Normal Galaxies
- Towards an Understanding of the Mid-Infrared Surface Brightness of Normal Galaxies
- ISO observations of Hickson Compact Group 31 with the central Wolf-Rayet galaxy NGC 1741
- ISO observations of the interacting galaxy Markarian 297: with the powerful supernova remnant 1982aa