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Synthetic light curve analysis of the close binary systems BX Andromedae and RR Leporis

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Abstract

Unpublished photoelectric observations of the systems BX And and RR Lep were subjected to light curve analysis using the Wilson-Devinney Code.

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Authors and Affiliations

  1. J. I. Holcomb Observatory Butler University, 46208, Indianapolis, IN

    R. E. Fuller

  2. Department of Astronomy, Ohio State University, 43210-1106, Columbus, OH

    R. H. Kaitchuck

  3. Department of Physics and Astronomy, Clemson University, 29634-1911, Clemson, SC

    B. B. Bookmyer

  4. Department of Math and Sciences, U. So. Carolina at Lancaster, 29720, Lancaster, SC, USA

    D. R. Faulkner

Authors
  1. R. G. Samec
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  2. R. E. Fuller
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  3. R. H. Kaitchuck
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  4. B. B. Bookmyer
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  5. D. R. Faulkner
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Additional information

Visiting Astronomer, Cerro Tololo Inter-American Observatories, National Optical Astronomy Observatories, operated by the Association of Universities for Research in Astronomy, Inc., under contract with the National Science Foundation.

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Samec, R.G., Fuller, R.E., Kaitchuck, R.H. et al. Synthetic light curve analysis of the close binary systems BX Andromedae and RR Leporis. Space Sci Rev 50, 359–360 (1989). https://doi.org/10.1007/BF00215964

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  • DOI: https://doi.org/10.1007/BF00215964

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