No CrossRef data available.
Article contents
Emission-like feature due to a latitudinal differential rotation
Published online by Cambridge University Press: 26 May 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.
We simulate the effect due to a latitudinal differential rotation on a HeI λ4471 absorption line. The effect can produce an emission-like reversal in the line core.
- Type
- 5. Be Stars: Spectroscopy and Photometry
- Information
- Copyright
- Copyright © Kluwer 1994
References
Baade, D.: 1990, in Wilson, L.A. and Stalio, R., ed(s).,
Angular Momentum and Mass Loss for Hot Stars
, Kluwer Acad. Publ., 177
Google Scholar