Ages for illustrative groups of field stars via gyrochronology

Details Ages for illustrative groups of field stars via gyrochronology Ages for illustrative groups of field stars via gyrochronology

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aas...207.6911b&link_type=abstract

American Astronomical Society Meeting 207, #69.11; Bulletin of the American Astronomical Society, Vol. 37, p.1272

Astronomy and Astrophysics

Astronomy

Scientific paper

Gyrochronology is the technique of deriving ages for solar- and late-type main sequence stars using their rotation periods and colors. This technique is clarified and developed here, and used to derive ages for illustrative groups of nearby, late-type, and some individual field stars with known rotation periods. (NSF is gratefully acknowledged for support of this work).

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