Abstract
Asymmetries in exoplanet transits are a useful tool for developing our understanding of magnetic activity on both stars and planets outside our Solar System. Near-UV observations of the WASP-12 system have revealed asymmetries in the timing of the transit when compared with the optical light curve. In this proceedings we review a number of reported asymmetries and present work simulating near-UV transits for the hot-Jupiter hosting star HD 189733. © International Astronomical Union 2014.
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Llama, J., Vidotto, A. A., Jardine, M., Wood, K., & Fares, R. (2014). Bow shocks and winds around HD 189733b. Proceedings of the International Astronomical Union, 9(S302), 245–246. https://doi.org/10.1017/S1743921314002191
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