Hans Publishers, Astronomy & Astrophysics, 1(474), p. 165-168
DOI: 10.1051/0004-6361:20078039
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The active K1 giant sigma Gem and its differential surface rotation is revisited. We refine our previous inconclusive result by recovering the spot migration pattern of this long-period RS CVn-type binary through application of the technique of ``average cross-correlation of contiguous Doppler images'' to a set of six Doppler images from 3.6 consecutive rotation cycles. We find an anti-solar differential rotation law with a shear of alpha≈ -0.022±0.006. We also find evidence of a poleward migration trend of spots with an average velocity of ≈300 m s-1.