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The Shocking Variability Of Exoplanet Transits

Published online by Cambridge University Press:  06 January 2014

J. Llama ,
A. A. Vidotto ,
M. Jardine ,
K. Wood  and
R. Fares
J. Llama
Affiliation:
SUPA. University of St Andrews. North Haugh. St Andrews. KY16 9SS. UK email: joe.llama@st-andrews.ac.uk
A. A. Vidotto
Affiliation:
SUPA. University of St Andrews. North Haugh. St Andrews. KY16 9SS. UK email: joe.llama@st-andrews.ac.uk
M. Jardine
Affiliation:
SUPA. University of St Andrews. North Haugh. St Andrews. KY16 9SS. UK email: joe.llama@st-andrews.ac.uk
K. Wood
Affiliation:
SUPA. University of St Andrews. North Haugh. St Andrews. KY16 9SS. UK email: joe.llama@st-andrews.ac.uk
R. Fares
Affiliation:
SUPA. University of St Andrews. North Haugh. St Andrews. KY16 9SS. UK email: joe.llama@st-andrews.ac.uk
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Abstract

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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

stars: activitycoronaeindividual (WASP-12, HD 189733)magnetic fieldsplanetary systemswinds
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S299: Exploring the Formation and Evolution of Planetary Systems , June 2013 , pp. 262 - 265
Copyright
Copyright © International Astronomical Union 2013 

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