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BV photometry of the RRc variable star DH Pegasi

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Abstract

Revised light elements of the RR Lyrae variable star DH Pegasi are presented together with a newBV light curve.

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References

  • Fitch, W. S., Wiśniewski, W. Z. and Johnson, H. L.: 1966,Comm. Lunar Planetary Lab. 71, 3.

    Google Scholar 

  • Geyer, E. H.: 1961,Z. Astrophys. 52, 229.

    Google Scholar 

  • Paczynski, B.: 1965,Acta Astron. 15, 115.

    Google Scholar 

  • Spinrad, H.: 1959,Astrophys. J. 130, 539.

    Google Scholar 

  • Szeidl, B.: 1975, in W. S. Fitch (ed.),Multiple Period Variable Stars, D. Reidel Publishing Co., Dordrecht, Holland, p. 135.

    Google Scholar 

  • Tifft, W. G.: 1964,Astrophys. J. 139, 451.

    Google Scholar 

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Authors and Affiliations

  1. Wilhelm Foerster Sternwarte, Berlin, FRG

    U. Hopp

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  1. U. Hopp
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Hopp, U. BV photometry of the RRc variable star DH Pegasi. Astrophys Space Sci 79, 239–242 (1981). https://doi.org/10.1007/BF00655920

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  • DOI: https://doi.org/10.1007/BF00655920

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