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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

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