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Long-Term Variability in the Winds of λ Eridani and 66 Ophiuchi

Published online by Cambridge University Press:  12 April 2016

Geraldine J. Peters*
Affiliation:
Space Sciences Center, University of Southern California, Los Angeles, CA 90089-1341, USA

Abstract

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Variations in the winds of the Be stars λ Eri and 66 Oph during the lifetime of the IUE spacecraft and the response of the Hα-emitting disk to these changes are briefly discussed. Common behavior is identified and evidence for cyclical variability on a time scale of ∼1 yr is presented.

Type
3. Periodic Variations
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Grady, C.A., Sonneborn, G., Wu, C.-C., & Henrichs, H. 1987, ApJS 65, 673 Google Scholar
Mennickent, R.E., Sterken, C., & Vogt, N. 1998, A&A 330, 631 Google Scholar
Peters, G.J. 1988, PASP 100, 207 CrossRefGoogle Scholar
Peters, G.J. 1998, in ESO Astrophys. Symp., Cyclical Variations in Stellar Winds, ed. Kaper, L. & Fullerton, A. (Berlin: Springer), 127 CrossRefGoogle Scholar
Scargle, J.D. 1982, ApJ 263, 835 Google Scholar
Smith, M.A. 1989, ApJS 71, 357 Google Scholar