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Detection of an x-ray flare from a single G dwarf star

  • B.C. Monsignori-Fossi
  • R. Pallavicini
  • M. Landini
  • L. Piro
Session III: Small Scale Atmosphere Structures: Data
Part of the Lecture Notes in Physics book series (LNP, volume 254)

Keywords

Solar Flare Dwarf Star Hardness Ratio Flare Star High Rotation Rate 
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. Haisch, B.M. (1983) in Activity in Red-dwarfs Stars (P.B. Byrne and M. Rodonb eds.), p. 255.Google Scholar
  2. Linsky, J.L., Worden, S.P., McClintock, W. and Robertson, R.M. (1979) Astrophys. J. Suppl. 41, 47.CrossRefGoogle Scholar
  3. Pallavicini, R., Monsignori-Fossi, B.C. and Landini, M. (1985), this volume.Google Scholar
  4. Pallavicini, R., Serio, S. and Vaiana, G.S. (1977) Astrophys. J. 216, 108.CrossRefGoogle Scholar
  5. Vaiana, G.S. et al. (1981) Astrophys. J. 245, 163.CrossRefGoogle Scholar
  6. White, N.E., Culhane, J.L., Parmar, A.N., Kellet, B., Kahn, S., van den Oort, G.H.J. and Kuipers, J. (1985) Astrophys. J., in press.Google Scholar

Copyright information

© Springer-Verlag 1986

Authors and Affiliations

  • B.C. Monsignori-Fossi
    • 1
  • R. Pallavicini
    • 1
  • M. Landini
    • 1
  • L. Piro
    • 2
  1. 1.Arcetri ObservatoryFlorenceItaly
  2. 2.TE.S.R.E. InstituteBolognaItaly

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