Visual observations of the semiregular variable UU Her in 1978 - 1979 are presented. A period of 80.1 days is determined from the analysis of the light curve by the method of Jurkevich (1971). A light curve has some RV Tauri features, but is as a whole peculiar. UU Her can hardly be classified as a cepheid or a typical SRd-variable if all available facts are considered.
Peremennye Zvezdy Prilozhenie
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