The Impact of Galaxy Formation on the Diffuse Background Radiation
The far infrared background is a sink for the hidden aspects of galaxy formation. At optical wavelengths, ellipticals and spheroids are old, even at $z \sim 1.$ Neither the luminous formation phase nor their early evolution is seen in the visible. We infer that ellipticals and, more generally, most...
| Asıl Yazarlar: | , |
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| Materyal Türü: | Conference item |
| Baskı/Yayın Bilgisi: |
2000
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