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S. A. Barnes (Univ. of Wisconsin-Madison)
Rotation measurements of young main-sequence stars suggest a large range in rotation created by processes on the pre-main sequence. I will summarize and review these observations, as revealed by measurements in a series of open clusters, and draw attention to some deficiencies in the available dataset. Finally, I will also discuss the validity of some of the current beliefs in rotational evolution beyond the early stages.
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Bulletin of the American Astronomical Society, 34
© 2002. The American Astronomical Soceity.