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Ultraviolet properties of the symbiotic stars

Published online by Cambridge University Press:  12 April 2016

Mark H. Slovak  and
David L. Lambert
Mark H. Slovak
Affiliation:
University of Texas at Austin, U.S.A.
David L. Lambert
Affiliation:
University of Texas at Austin, U.S.A.

Extract

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Prior to the launch of the IDE satellite in early 1978, the only symbiotic star previously detected in the ultraviolet by earlier UV satellites, such as the 0A0-2, TD-1 and ANS experiments, was AG Pegasi = HD 207757 (Gallager et al. 1979). These broad-band observations indicated that the symbiotics as a class may show a significant ultraviolet flux and thus they became natural candidates for a survey with the IUE satellite. The following is an interim report on a survey of the symbiotics, both at low and, for AG Pegasi and CH Cygni, at high resolution.

Type
Session I - New Observations of Symbiotic Stars
Information
International Astronomical Union Colloquium , Volume 70: The Nature of Symbiotic Stars , 1982 , pp. 103 - 113
Copyright
Copyright © Reidel 1982

References

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