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Radio observations of active stars: Direct evidence for polarity reversals?

  • D. M. Gibson
2. Rotation and Activity in Main Sequence Stars
Part of the Lecture Notes in Physics book series (LNP, volume 193)

Keywords

Radio Emission Circular Polarization Active Star Coherent Emission Spectroscopic Binary 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. Fisher, P. L. and Gibson, D. M. 1982, in Second Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun (SAO Spec. Rept. 392), eds. M. S. Giampapa and L. Golub, Vol. 2, p. 109.Google Scholar
  2. Gibson, D. M. 1983, Proc. Southwest Reg. Conf. Astron. Astrophys., IX, in press.Google Scholar
  3. Hjellming, R. M. and Gibson, D. M. 1980, in Radio Physics of the Sun, IAU Symp. 86, eds. M. R. Kundu and T. E. Gergely (Dordrecht: Reidel), p. 209.Google Scholar
  4. Melrose, D. B. and Dulk, G. A. 1982, Ap. J., 259, 844.CrossRefGoogle Scholar
  5. Owen, F. N., Jones, T. W., and Gibson, D. M. 1976, Ap. J. (Lett.), 210, L27.CrossRefGoogle Scholar
  6. Spangler, S. R. 1977, A. J., 82, 169.CrossRefGoogle Scholar
  7. Stenflo, J. O. 1968, in Structure and Development of Solar Active Regions, IAU Symp. 3, ed. H. Kiepenheuer (Dordrecht: Reidel), p. 47.Google Scholar

Copyright information

© Springer-Verlag 1984

Authors and Affiliations

  • D. M. Gibson
    • 1
  1. 1.Joint Institute for Laboratory AstrophysicsUniversity of Colorado and National Bureau of StandardsBoulder

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