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Rotation among solar-type starsThe 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.
Document ID
19950008092
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Soderblom, D. (Space Telescope Science Inst. Baltimore, MD, United States)
Date Acquired
September 6, 2013
Publication Date
August 1, 1994
Publication Information
Publication: NASA. Ames Research Center, Astrophysical Science with a Spaceborne Photometric Telescope
Subject Category
Astrophysics
Accession Number
95N14506
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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