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Intensifier-Dissector-Scanner Observations of the Bright Northern Be Stars

Published online by Cambridge University Press:  14 August 2015

Paul K. Barker
Paul K. Barker*
Affiliation:
The University of Western Ontario

Abstract

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Early results are presented from an extensive program of regular Balmer-line spectroscopy; during eight months in 1980 Hα profiles were obtained of over 100 northern Be stars. Transient emission events have been observed in the very early rapid rotator 59 Cygni; sequential variations in Hα are quasi-periodic.

Type
III. Spectroscopy
Information
Symposium - International Astronomical Union , Volume 98: Be Stars , 1982 , pp. 147 - 150
Copyright
Copyright © Reidel 1982 

References

Barker, P.K. 1980, IAU Circ. No. 3498.Google Scholar
Barker, P.K. 1981, preprint.Google Scholar
Doazan, V., Kuhi, L., and Thomas, R.N. 1980, Astrophys. J. Letters, 235, L17.Google Scholar
Hubert-Delplace, A.-M., and Hubert, H. 1979, “An Atlas of Be Stars”, Paris-Meudon Observatory.Google Scholar
Hutchings, J.B. 1970, Monthly Notices Roy. Astron. Soc., 150, p. 55.CrossRefGoogle Scholar
Marlborough, J.M., and Snow, T.P. 1980, Astrophys. J., 235, p. 85.Google Scholar
Tomaszewski, L. 1980, , The University of Western Ontario.Google Scholar
Tomaszewski, L., Symonds, G.R., and Landstreet, J.D. 1980, Publ. Astron. Soc. Pacific, 92, p. 518.Google Scholar