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UW Persei |
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| Authors: | G A Richter |
| Abstract: | This object consists of two visible components; it is not quite sure if the brighter one is variable. An examination on 314 plates gave no further maximum in addition to the three already known historical eruptions. A relationship of the brighter component to the cataclysmic variables is not very probable because of the observed UV weakness. |
| Keywords: | variables eruptive binaries photographic observations light variations |