@inproceedings{0d81e0d466184454b705524bd1d2afb8,
title = "The shocking variability of exoplanet transits",
abstract = "Asymmetries in exoplanet transits are proving to be a useful tool for furthering 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 paper we review a number of reported asymmetries and present work simulating near-UV transits for the hot-Jupiter hosting star HD 189733.",
keywords = "Coronae, Individual (WASP-12, HD 189733), Magnetic fields, Planetary systems, Stars: activity, Winds",
author = "J. Llama and Vidotto, {A. A.} and M. Jardine and K. Wood and R. Fares",
year = "2013",
doi = "10.1017/S1743921313008521",
language = "English",
isbn = "9781107045200",
volume = "8",
series = "Proceedings of the International Astronomical Union",
publisher = "Cambridge University Press",
number = "S299",
pages = "262--265",
booktitle = "Exploring the Formation and Evolution of Planetary Systems",
address = "United Kingdom",
edition = "S299",
}