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Detection of co emission in hydra 1 cluster galaxies
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Huchtmeier, W. K. |
| Copyright Year | 1990 |
| Description | A survey of bright Hydra cluster spiral galaxies for the CO(1-0) transition at 115 GHz was performed with the 15m Swedish-ESO submillimeter telescope (SEST). Five out of 15 galaxies observed have been detected in the CO(1-0) line. The largest spiral galaxy in the cluster, NGC 3312, got more CO than any spiral of the Virgo cluster. This Sa-type galaxy is optically largely distorted and disrupted on one side. It is a good candidate for ram pressure stripping while passing through the cluster's central region. A comparison with global CO properties of Virgo cluster spirals shows a relatively good agreement with the detected Hydra cluster galaxies. |
| File Size | 228767 |
| Page Count | 3 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19910004924 |
| Archival Resource Key | ark:/13960/t7rn82j04 |
| Language | English |
| Publisher Date | 1990-07-01 |
| Access Restriction | Open |
| Subject Keyword | Astrophysics Surveys Galactic Clusters Virgo Galactic Cluster Telescopes Submillimeter Waves Emission Distortion Spiral Galaxies Carbon Monoxide Detection Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
