OPTICAL LINE EMISSION IN BRIGHTEST CLUSTER GALAXIES AT 0 < z < 0.6: EVIDENCE FOR A LACK OF STRONG COOL CORES 3.5 Gyr AGO?
In recent years the number of known galaxy clusters beyond z gsim 0.2 has increased drastically with the release of multiple catalogs containing >30,000 optically detected galaxy clusters over the range 0 < z < 0.6. Combining these catalogs with the availability of optical spectroscopy of t...
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| Format: | Article |
| Language: | English |
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Institute of Physics/American Astronomical Society,
2015-03-04T19:28:06Z.
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| Online Access: | Get fulltext |