High-redshift galaxy populations |
| |
Authors: | Hu Esther M Cowie Lennox L |
| |
Affiliation: | Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, Hawaii 96822, USA. hu@ifa.hawaii.edu |
| |
Abstract: | ![]() We now see many galaxies as they were only 800 million years after the Big Bang, and that limit may soon be exceeded when wide-field infrared detectors are widely available. Multi-wavelength studies show that there was relatively little star formation at very early times and that star formation was at its maximum at about half the age of the Universe. A small number of high-redshift objects have been found by targeting X-ray and radio sources and most recently, gamma-ray bursts. The gamma-ray burst sources may provide a way to reach even higher-redshift galaxies in the future, and to probe the first generation of stars. |
| |
Keywords: | |
本文献已被 PubMed 等数据库收录! |
|