Abstract
Results of submillimeter observations of the very high-redshift IRAS
galaxy 10214 + 4724 are presented. Significant detections at 800 and 450
are achieved. The data are compared to the existing models of this
galaxy, and it is found that both the extreme primeval galaxy model an
the dust-embedded Seyfert model are excluded. The galaxy is likely to be
undergoing and extreme starburst, but whether this represents the
formation of a significant fraction of the stars is unclear.
Original language | English |
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Pages (from-to) | 349 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 256 |
DOIs | |
Publication status | Published - 1 May 1992 |
Keywords
- Galactic Evolution
- Galactic Radio Waves
- Infrared Astronomy
- Starburst Galaxies
- Submillimeter Waves
- Far Infrared Radiation
- Infrared Astronomy Satellite
- Red Shift