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Photometric variability of main-sequence stars from Wilson's survey

  • Session I: Dynamos and Stellar Activity: Observations
  • Conference paper
  • First Online:
Cool Stars, Stellar Systems, and the Sun

Part of the book series: Lecture Notes in Physics ((LNP,volume 254))

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References

  • Duncan, D. K., Baliunas, S. L.,Noyes, R. W.,Vaughan, A. H., Frazer, J., and Lanning, H. H. (1984). Publ. Astron. Soc. Pacific 96, 707.

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  • Lockwood, G. W., and Skiff, B. A. (1985). Submitted to Publ. Astron. Soc. Pacific.

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  • Lockwood, G. W., Thompson, D. T., Radick, R. R., Osborn, W. H., Baggett, W. E., Duncan, D. K., and Hartmann, L. W. (1984). Publ. Astron. Soc. Pacific 96, 714.

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Authors and Affiliations

  1. Lowell Observatory, Mars Hill Road, 1400 West Flagstaff, 86001, Arizona

    G. W. Lockwood & Brian A. Skiff

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  1. G. W. Lockwood
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  2. Brian A. Skiff
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Michael Zeilik David M. Gibson

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© 1986 Springer-Verlag

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Lockwood, G.W., Skiff, B.A. (1986). Photometric variability of main-sequence stars from Wilson's survey. In: Zeilik, M., Gibson, D.M. (eds) Cool Stars, Stellar Systems, and the Sun. Lecture Notes in Physics, vol 254. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-16763-3_141

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  • DOI: https://doi.org/10.1007/3-540-16763-3_141

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-16763-1

  • Online ISBN: 978-3-540-38731-2

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