No CrossRef data available.
Article contents
Long-Term Variability in the Winds of λ Eridani and 66 Ophiuchi
Published online by Cambridge University Press: 12 April 2016
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
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
- Information
- International Astronomical Union Colloquium , Volume 175: The Be Phenomenon in Early-Type Stars , 2000 , pp. 212 - 215
- Copyright
- Copyright © Astronomical Society of the Pacific 2000
References
Peters, G.J.
1998, in ESO Astrophys. Symp., Cyclical Variations in Stellar Winds, ed. Kaper, L. & Fullerton, A. (Berlin: Springer), 127
CrossRefGoogle Scholar
You have
Access