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Co deficiency in galaxies of the fornax cluster?
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Casoli, Fabienne Horellou, Cathy Dupraz, Christophe |
| Copyright Year | 1993 |
| Description | There is ample observational evidence that cluster galaxies are different from those in the field. Interaction with the hot intracluster medium affects the morphology of the galaxies, their gaseous content and possibly their star-formation activity. Tidal encounters between galaxies also play an important role. The atomic component has been investigated in detail for several clusters, among them our neighbor Virgo. With the Swedish-ESO 15 m telescope, we have observed in the 12CO(1-0) transition the 23 brightest spirals and lenticulars of the Formax cluster. |
| File Size | 136692 |
| Page Count | 2 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19930017602 |
| Archival Resource Key | ark:/13960/t8z945462 |
| Language | English |
| Publisher Date | 1993-01-01 |
| Access Restriction | Open |
| Subject Keyword | Astrophysics Galactic Clusters Star Formation Galaxies Rotational Spectra Morphology Encounters Tides Ntrs Nasa Technical Reports ServerĀ (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |