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Scanner observations of shell stars Phi Persei and Psi Persei
Spectrophotometric energy distribution data of the shell stars Phi Perand Psi Per are reported in the wavelength range 3200-8000 A. Theeffective temperature of these stars is derived by comparison ofobserved energy distribution with theoretical models. Both the starsshow higher values of derived effective temperature. The continuumenergy distribution in the ultraviolet region has also been discussed.
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