The Differential Rotation Profile of kappa1 Ceti from MOST Photometry

Details The Differential Rotation Profile of kappa1 Ceti from MOST Photometry The Differential Rotation Profile of kappa1 Ceti from MOST Photometry

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...209.1401w&link_type=abstract

2007 AAS/AAPT Joint Meeting, American Astronomical Society Meeting 209, #14.01; Bulletin of the American Astronomical Society, V

Astronomy and Astrophysics

Astronomy

Scientific paper

The nearby G5 V star, kappa1 Ceti, has a differential rotation profile
closely ressembling that for the Sun, despite rotating nearly three time
faster. This conclusion is based on the different rotation periods of
star spots detected over a wide range of latitudes in MOST satellite
light curves from 2003, 2004 and 2005.

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