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Possibilities and Attempts to Determine the Differential Rotation on F-Type Main-Sequence Stars
Published online by Cambridge University Press: 04 August 2017
Abstract
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A preliminary analysis of spectral lines by Fourier transformation was used to determine upper limits of differential rotation for 11 F-type stars, mainly from the main-sequence. No evidence for a much steeper differential rotation on these stars than on the Sun could be found.
- Type
- II. Rotation — Activity — Cycle — Age Connection: Observations
- Information
- Copyright
- Copyright © Reidel 1983
References
Uesugi, A.: 1976, Revised Catalogue of Stellar Rotational Velocities (Kyoto: University of Kyoto Press).Google Scholar
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