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A companion quasar to 3C345
Although some quasistellar objects (QSOs) are known to be members of small groups of galaxies (see refs 1–3), there is no known case of a QSO in a rich cluster of galaxies 4 . Whether this has important implications for the nature of QSOs, or is simply a reflection of the difficulty of observing hig...
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Published in: | Nature (London) 1981-04, Vol.290 (5806), p.480-481 |
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Main Authors: | , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | Although some quasistellar objects (QSOs) are known to be members of small groups of galaxies (see refs 1–3), there is no known case of a QSO in a rich cluster of galaxies
4
. Whether this has important implications for the nature of QSOs, or is simply a reflection of the difficulty of observing high-redshift clusters, is unclear. Here we report the discovery of a new QSO which provides perhaps the strongest evidence to date for quasar membership in a rich cluster. |
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ISSN: | 0028-0836 1476-4687 |
DOI: | 10.1038/290480a0 |