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D. M. Terndrup (Ohio State University)
I will review recent progress in the observations and theory of stellar angular momentum evolution in clusters and groups with ages up to that of the Hyades. Along the way, I will attempt to identify a few areas where we may be able to make observational breakthroughs in the near future. I will close by proposing ways to determine whether environmental effects matter in the initial angular momentum distribution in young systems.
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Bulletin of the American Astronomical Society, 34
© 2002. The American Astronomical Soceity.