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X-Ray Detection of the Symbiotic Star AG Draconis

  • Christopher M. Anderson
  • Joseph P. Cassinelli
  • Nancy A. Oliversen
  • Roy V. Myers
  • W. T. Sanders
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 95)

Abstract

The symbiotic star AG Draconis was observed by the HEAO-2 Imaging Proportional Counter (IPC) and found to be an unusually intense source of very soft X-rays.

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References

  1. Anderson, C. M., Cassinelli, J. P. and Sanders, W. T. 1981, Ap.J. 247, L127.ADSCrossRefGoogle Scholar
  2. Brown, R. L. and Gould, J. R. 1970, Phys. Rev. D, 3d Ser., 1, 2252.Google Scholar
  3. Heiles, C. 1974 Astr. Ap. Supl., 20, 37.ADSGoogle Scholar
  4. Lampton, M, Margon, B., and Boyer, S 1976, Ap.J., 208, 177.ADSCrossRefGoogle Scholar
  5. Nordsieck, K. H., Cassinelli, J. P. and Anderson, C. M. 1981, Ap.J. 248, 678.ADSCrossRefGoogle Scholar
  6. Raymond, J. C. ana Smith B. W. 1979, private communication.Google Scholar

Copyright information

© D. Reidel Publishing Company, Dordrecht, Holland 1982

Authors and Affiliations

  • Christopher M. Anderson
    • 1
  • Joseph P. Cassinelli
    • 1
  • Nancy A. Oliversen
    • 1
  • Roy V. Myers
    • 1
  • W. T. Sanders
    • 2
  1. 1.Washburn ObservatoryUniversity of Wisconsin-MadisonUSA
  2. 2.Department of PhysicsUniversity of Wisconsin-MadisonUSA

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