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X-ray selected M-dwarfs and the diffuse X-ray background

  • Jean-Pierre Caillault
  • David J. Helfand
  • John A. Nousek
  • Leo O. Takalo
Session I: Dynamos and Stellar Activity: Observations
Part of the Lecture Notes in Physics book series (LNP, volume 254)

Keywords

Thermal Model Luminosity Function High Luminosity Candidate Object Sloan Foundation 
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. Cox, D. P. and Anderson, P. R. 1982, Ap. J., 253, 268.CrossRefGoogle Scholar
  2. Fried, P. M., Nousek, J. A., Sanders, W. T., and Kraushaar, W. L. 1980, Ap. J., 242, 987.CrossRefGoogle Scholar
  3. Raymond, J. C. and Smith, B. W. 1977, Ap. J. Suppl., 35, 419.CrossRefGoogle Scholar
  4. Rosner, R. et al. 1981, Ap. J. (Letters), 249, L5.CrossRefGoogle Scholar
  5. Rosner, R., Golub, L., and Vaiana, G. S. 1985, Ann. Rev. Astr. Ap., 23, XXX.Google Scholar

Copyright information

© Springer-Verlag 1986

Authors and Affiliations

  • Jean-Pierre Caillault
    • 1
  • David J. Helfand
    • 1
  • John A. Nousek
    • 2
  • Leo O. Takalo
    • 2
  1. 1.Columbia Astrophysics LaboratoryColumbia UniversityUSA
  2. 2.Department of AstronomyPennsylvania State UniversityUSA

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