Magnetic cycles of the planet-hosting star tauBootis
J. F. Donati, C. Moutou, R. Fares, D. Bohlender, C. Catala, M., Deleuil, E. Shkolnik, A. C. Cameron, M. M. Jardine, G. A. H. Walker

TL;DR
This study confirms tauBootis has a magnetic cycle with polarity reversals, exhibits strong differential rotation, and suggests the planet's tidal influence may synchronize stellar rotation with its orbit, affecting magnetic activity.
Contribution
First observation of a global magnetic polarity switch in a star other than the Sun, linking differential rotation and magnetic cycle period in tauBootis.
Findings
Magnetic polarity reversed, indicating a magnetic cycle.
Differential rotation is 6-10 times stronger than the Sun's.
Star's rotation is synchronized with its planet's orbit.
Abstract
We have obtained new spectropolarimetric observations of the planet-hosting star tauBootis, using the ESPaDOnS and NARVAL spectropolarimeters at the Canada-France-Hawaii Telescope and Telescope Bernard-Lyot. With this data set, we are able to confirm the presence of a magnetic field at the surface of tauBoo and map its large-scale structure over the whole star. The overall polarity of the magnetic field has reversed with respect to our previous observation (obtained a year before), strongly suggesting that tauBoo is undergoing magnetic cycles similar to those of the Sun. This is the first time that a global magnetic polarity switch is observed in a star other than the Sun; we speculate that the magnetic cycle period of tauBoo is much shorter than that of the Sun. Our new data also allow us to confirm the presence of differential rotation from the latitudinal shearing that the magnetic…
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