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SB 939 - A New Intermediate Helium Star at High Galactic Latitudes

Published online by Cambridge University Press:  12 April 2016

G. Langhans
Affiliation:
Institut für Theoretische PhysikundSternwarte der UniversitätKiel Olshausenstr. 40, 2300 Kiel, F.R.G.
U. Heber
Affiliation:
Institut für Theoretische PhysikundSternwarte der UniversitätKiel Olshausenstr. 40, 2300 Kiel, F.R.G.

Abstract

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SB 939 was analyzed spectroscopically for the basic atmospheric parameters Teff, log g and helium content. It was shown to be an intermediate helium star (helium abundance = 22% by number) situated unusually far away from star-forming regions.

Type
VI Intermediate Helium Stars
Copyright
Copyright © Reidel 1986

References

Blaauw, A.: 1961, Bull. Astron. Inst. Neth. 15, 265 Google Scholar
Graham, J.A. and Slettebak, A.: 1973, Astron. J. 78, 295 CrossRefGoogle Scholar
Hejlesen, P.M: 1980, Astron: Astrophys. Suppl. 39, 347 Google Scholar
Kurucz, R.L.: 1979, Astrophys. J., Suppl. 40, 1 CrossRefGoogle Scholar
Slettebak, A., Brundage, R.K: 1971, Astron. J. 76, 338 Google Scholar
Walborn, N.R.: 1983, Astrophys. J. 268, 195 Google Scholar