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Absolute Spectrophotometry of Be Stars

Published online by Cambridge University Press:  23 September 2016

T. Stiff  and
S. Jeffers
T. Stiff
Affiliation:
Cress, York University, Canada
S. Jeffers
Affiliation:
Department of Physics, York University, Canada

Abstract

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Absolute spectrophotometry data have been obtained for a sample of Be stars. These data were obtained with the York Observatory 60 cm telescope and vidicon spectrophotometer. The data have been corrected for differential atmospheric extinction, instrumental response, and interstellar extinction and calibrated in terms of absolute flux. Absolute Hα and Hβ fluxes have been determined.

Type
III. The Circumstellar Gas
Information
International Astronomical Union Colloquium , Volume 92: Physics of Be Stars , August 1987 , pp. 211 - 213
Copyright
Copyright © Cambridge University Press 1987

References

Breger, (1976), Astrophysical Journal Supp. 32, p. 1.CrossRefGoogle Scholar
Jeffers, , Stiff, , Weller, (1983), Proceeding of S.P.I.E. 445, p. 199 Google Scholar
Lamers, & Snow, (1978), Astrophysical Journal 219, p. 504.CrossRefGoogle Scholar
Lesh, (1968), Astrophysical Journal Supp. 17, p. 371.CrossRefGoogle Scholar
Seaton, (1970), Mon. Not. R. Astron. Soc. 187, p. 73.CrossRefGoogle Scholar
Weller, , Herbst, , Jeffers, (1977), Pub. Astron. Soc. Pacific 89, p. 935.CrossRefGoogle Scholar