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Periodic variations in the IUE data of HD 50896

Published online by Cambridge University Press:  07 August 2017

C. Lloyd  and
D. J. Stickland
C. Lloyd
Affiliation:
Rutherford Appleton Laboratory, Chilton, U.K.
D. J. Stickland
Affiliation:
Rutherford Appleton Laboratory, Chilton, U.K.

Abstract

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A periodogram analysis of the radial velocities and absorption line strengths from IUE spectra of HD 50896 show evidence of the 3.766 day period usually associated with this star. The dominant line variations occur on time scales of ∼ 1 day but may be interpreted as higher order harmonics of the 3.766 day period.

Keywords

stars: Wolf-Rayetvariableindividual: HD 50896
Type
Session I - Basic parameters, properties of single Wolf-Ray et stars
Information
Symposium - International Astronomical Union , Volume 163: Wolf-Rayet Stars: Binaries, Colliding Winds, Evolution , 1995 , pp. 58 - 59
Copyright
Copyright © Kluwer 1995 

References

Antokhin, I., Bertrand, J-F., Lamontagne, R., Moffat, A.F.J. 1994, AJ 107, 2179 Google Scholar
St-Louis, N.S., Howarth, I.D., Willis, A.J., Stickland, D.J, Smith, L.J., Conti, P.S., Garmany, C.D. 1993, A&A 267, 449 Google Scholar
Willis, A.J., Howarth, I.D., Smith, L.J., Conti, P.S., Garmany, C.D. 1989, A&A Suppl. 77, 269 Google Scholar