Hostname: page-component-78c5997874-mlc7c Total loading time: 0 Render date: 2024-11-20T03:39:00.542Z Has data issue: false hasContentIssue false
  • English
  • Français

X-ray detection of the symbiotic star AG Draconis

Published online by Cambridge University Press:  12 April 2016

Christopher M. Anderson ,
Joseph P. Cassinelli ,
Nancy A. Oliversen ,
Roy V. Myers  and
W.T. Sanders
Christopher M. Anderson
Affiliation:
Washburn Observatory, University of Wisconsin-Madison
Joseph P. Cassinelli
Affiliation:
Washburn Observatory, University of Wisconsin-Madison
Nancy A. Oliversen
Affiliation:
Washburn Observatory, University of Wisconsin-Madison
Roy V. Myers
Affiliation:
Washburn Observatory, University of Wisconsin-Madison
W.T. Sanders
Affiliation:
Department of Physics, University of Wisconsin-Madison

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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.

Type
Session I - New Observations of Symbiotic Stars
Information
International Astronomical Union Colloquium , Volume 70: The Nature of Symbiotic Stars , 1982 , pp. 117 - 121
Copyright
Copyright © Reidel 1982

References

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