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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S299(8), p. 262-265, 2013

DOI: 10.1017/s1743921313008521

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The Shocking Variability Of Exoplanet Transits

Journal article published in 2013 by J. Llama ORCID, A. A. Vidotto, M. Jardine, K. Wood, R. Fares
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

AbstractAsymmetries 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.

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