NASA NTRS · 19950008092
Rotation among solar-type stars
Abstract
The net result is that FRESIP will produce high quality rotational data for a large (and essentially volume-limited) sample of solar-type stars. Moreover, the observed slight changes in rotation period will indicate the nature and degree of differential rotation on those stars. Both parameters are central to our understanding of the evolution of the Sun.
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Soderblom, D.. 1994-08-01. Rotation among solar-type stars. https://ntrs.nasa.gov/citations/19950008092
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