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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

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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

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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