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Spectral classification of eclipsing binaries

Published online by Cambridge University Press:  04 August 2017

George W. Wolf  and
Janet T. Kern
George W. Wolf
Affiliation:
Department of Physics and Astronomy Southwest Missouri State University Springfield, Missouri 65804 U.S.A.
Janet T. Kern
Affiliation:
Department of Physics and Astronomy Southwest Missouri State University Springfield, Missouri 65804 U.S.A.

Abstract

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Approximately 375 classification spectra of 130 Southern Hemisphere eclipsing binary stars were obtained between 1978 and 1982 at Mt. John University Observatory, New Zealand using the 0.6 meter reflector, and at Cerro Tololo Inter-American Observatory, Chile using the 0.4, 0.6, 0.9, and 1.0 meter telescopes. The spectra have been classified by one of us (GWW) using a grid of standards obtained on the various spectrographs at each of the observatories. Since many of the spectra were taken during primary and secondary minima, it has been possible in many cases to classify separately each component in the binaries.

Type
III. Spectroscopic Research Programmes
Information
Symposium - International Astronomical Union , Volume 118: Instrumentation and Research Programmes for Small Telescopes , 1986 , pp. 463 - 464
Copyright
Copyright © Reidel 1986 

References

Hilditch, R.W. and Hill, G. 1975, Mem. R. Astr. Soc. 79, 101 Google Scholar
Hill, G., Hilditch, R.W., Younger, F., and Fisher, W.A. 1975, Mem. R. Astr. Soc. 79, 131 Google Scholar
Wolf, G.W. and Kern, J.T. 1983, Astroph. J. Suppl. 52, 429 Google Scholar