HR7308 - a Short-Period Cepheid with Variable Amplitude

Physics

Scientific paper

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Scientific paper

HR 7308 is a F6 Ib-II star of 6th magnitude. Semi-regular
photometric variations were detected by Breger (1969), Percy et al.
(1979) find that this star is a new small-amplitude Cepheid, and Burki
and Mayor (1980) obtain a period of 1.49107 d. and detect a strongly
variable amplitude.

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