We present a new Doppler imaging study for the Li-rich single K-giant DI Psc. Surface temperature maps are reconstructed for two subsequent rotation cycles. From the time evolution of the spot distribution antisolar-type differential rotation pattern is revealed. We show marks of non-uniform Li-abundance as well. The possible connection between the current evolutionary phase of the star and its magnetic activity is briefly discussed. © International Astronomical Union 2014.
CITATION STYLE
Kriskovics, L., Kovári, Z., Vida, K., & Oláh, K. (2014). Activity on a Li-rich giant: Di Psc revisited. Proceedings of the International Astronomical Union, 9(S302), 383–384. https://doi.org/10.1017/S1743921314002567
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