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PULSATIONS OF LUMINOUS INTERMEDIATE-MASS STARS WITH APPLICATIONS TO UU HERCULIS

Pulsation models for the enigmatic F-type supergiant variable, UU Her are investigated. It is shown that irregular pulsations with small amplitude is realized, if UU her is assumed to be an intermediate mass F type supergiant star which has evolved with mass-loss and rotation mixing and thus highly luminous, compared with what is obtained by conventional evolution.