Using planetary transits to estimate magnetic cycles lengths in Kepler stars
Observations of various solar-type stars along decades showed that they could have magnetic cycles, just like our Sun. These observations yield a relation between the rotation period P rot and the cycle length P cycle of these stars. Two distinct branches for the cycling stars were identified: activ...
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Veröffentlicht in: | Proceedings of the International Astronomical Union 2016-10, Vol.12 (S328), p.152-158 |
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