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Ultraviolet Observations of 31 and 32 Cygni

Published online by Cambridge University Press:  14 August 2015

Robert E. Stencel ,
Yoji Kondo ,
Andrew P. Bernat  and
George McCluskey
Robert E. Stencel
Affiliation:
NASA - Goddard Space Flight Center
Yoji Kondo
Affiliation:
NASA - Goddard Space Flight Center
Andrew P. Bernat
Affiliation:
Kitt Peak National Observatory
George McCluskey
Affiliation:
Lehigh University

Extract

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Ultraviolet observations of the Zeta Aurigae systems appear to have several advantages over comparable visual wavelength studies. A wide range of large optical depth resonance lines of abundant species permit the study of the supergiant atmosphere and circumstellar environment at virtually all phases. The International Ultraviolet Explorer satellite (Boggess, et al., 1978) is well suited to obtaining spectra between 1150 and 3200 A, although the competition for observing time is non-negligible.

Type
X. … and The Rest (Symbiotics, Supergiants, Planetaries, Population II Systems)
Information
Symposium - International Astronomical Union , Volume 88: Close Binary Stars: Observations and Interpretation , 1980 , pp. 555 - 559
Copyright
Copyright © Reidel 1980 

References

Bernat, A., Stencel, R., Kondo, Y. and McCluskey, G., in preparation.Google Scholar
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