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Cool Stars, Stellar Systems, and the Sun pp 497–499Cite as

Spectral analysis of APT RS CVn binary light curves

  • Contributed Papers on Active Binary Stars
  • Conference paper
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Part of the book series: Lecture Notes in Physics ((LNP,volume 291))

Abstract

Preliminary analysis of U,B,V band RS CVn photometric data taken with the Automatic Photoelectric Telescope (Genet et. al., 1987) from the last quarter of 1983 to the first quarter of 1985 are presented. The fundamental photometric periods and V band amplitudes are tabulated and evidence for possible multiple periodic structure is discussed.

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Authors and Affiliations

  1. Science Applications, International Corporation, 4615 Hawkins NE, Albuquerque, NM

    Eric R. Nelson

  2. Institute for Astrophysics Department of Physics and Astronomy, University of New Mexico, 87106, Albuquerque, NM

    Eric R. Nelson

  3. Fairborn Observatory, 1357 N. 91st Place, 85207, Mesa, Arizona

    L. J. Boyd, R. M. Genet & D. S. Hall

Authors
  1. Eric R. Nelson
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  2. L. J. Boyd
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  3. R. M. Genet
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  4. D. S. Hall
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Editor information

Jeffrey L. Linsky Robert E. Stencel

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© 1987 Springer-Verlag

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Nelson, E.R., Boyd, L.J., Genet, R.M., Hall, D.S. (1987). Spectral analysis of APT RS CVn binary light curves. In: Linsky, J.L., Stencel, R.E. (eds) Cool Stars, Stellar Systems, and the Sun. Lecture Notes in Physics, vol 291. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-18653-0_183

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  • DOI: https://doi.org/10.1007/3-540-18653-0_183

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-18653-3

  • Online ISBN: 978-3-540-48041-9

  • eBook Packages: Springer Book Archive

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