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Hr 7308, a short period Cepheid with variable amplitude

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Abstract

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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Reference

  • Baranne, A., Mayor, M., Poncet, J.L., 1979, Vistas in Astronomy, 25, 279

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  • Breger, M., 1969, Astrophys. J. Suppl., 19, 79

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  • Burki, G., Mayor, M., 1980, Inf. Bull. Var. Stars 1728

  • Percy, J.R., Baskerville, I., Tremorrow, D.W., 1979, Publ. Astron. Soc. Pacific, 91, 368

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Authors and Affiliations

  1. Geneva Observatory, Switzerland

    G. Burki & M. Mayor

Authors
  1. G. Burki
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  2. M. Mayor
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Burki, G., Mayor, M. Hr 7308, a short period Cepheid with variable amplitude. Space Sci Rev 27, 429–430 (1980). https://doi.org/10.1007/BF00168330

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  • DOI: https://doi.org/10.1007/BF00168330

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