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IUE/OPTICAL/VLA flares on AD Leo

  • Dale E. Gary
  • P. B. Byrne
  • C. J. Butler
Nonthermal Phenomena in Stellar Coronae
Part of the Lecture Notes in Physics book series (LNP, volume 291)

Abstract

We discuss joint observations of flares on the dMe star AD Leo made with IUE, the VLA, and the Tinsley photometer at the University of Hawaii's 24-inch reflector on Mauna Kea. We find that optical emission is correlated with C IV while radio emission is better correlated with He II. We reach some tentative conclusions concerning timescales and source characteristics.

Keywords

Radio Emission Radio Source Line Flux Flare Star Very Large Array 
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. Avrett, E.H., Vernazza, J.E., Linsky, J.L. 1976, Ap. J. Lett., 207, L199.Google Scholar
  2. Ayres, T.R., Linsky, J.L., Brown, A., Jordan, C., Simon, T. 1982, Advances in Ultraviolet Astronomy: Four Years of IUE Research, NASA Conf. Publ. 2238 p281.Google Scholar
  3. Dulk, G.A. 1985, Ann. Rev. Astron. Ap., 23, 169.Google Scholar
  4. Lang, K.R., Bookbinder, J., Golub, L., Davis, M. 1983, Ap. J. Lett., 272, L15.Google Scholar
  5. Lang, K.R., Willson, R.F. 1986, Ap. J., 305, 363.Google Scholar

Copyright information

© Springer-Verlag 1987

Authors and Affiliations

  • Dale E. Gary
    • 1
  • P. B. Byrne
    • 2
  • C. J. Butler
    • 2
  1. 1.Pasadena
  2. 2.Armagh ObservatoryArmaghN. Ireland

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