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On the Rotation of A-Type Stars
Published online by Cambridge University Press: 12 April 2016
Abstract
Based upon the statistics of V sini among A-type stars it is shown that (1) no relationship exists between rotational velocity and UBV colours, (2) there might be an influence of rotation upon spectral classification, and (3) spectroscopic binaries are associated with low rotational velocity.
- Type
- Part III / Stellar Rotation in Binaries, Clusters, and Special Objects. Statistics of Stellar Rotation
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- Copyright
- Copyright © Reidel 1970