Paper:	Doppler Imaging of the RS CVn Binary IL Hydrae
Volume:	154, Cool Stars, Stellar Systems and the Sun: Tenth Cambridge Workshop
Page:	1366
Authors:	Weber, M.; Strassmeier, K. G.
Abstract:	We present preliminary results of a study linking rotational period to photospheric surface activity derived from Doppler images. New Doppler images of 15 stars of spectral classification G to K, luminosity class III to V and rotational periods of 1.5 to 25 days have been computed. These Doppler images - along with previously published material - were averaged into latitudinal strips and their temperature distribution correlated with evolutionary status and rotational period.

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