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.
| Original language | English |
|---|---|
| Title of host publication | Exploring the Formation and Evolution of Planetary Systems |
| Publisher | Cambridge University Press |
| Pages | 262-265 |
| Number of pages | 4 |
| Edition | S299 |
| ISBN (Print) | 9781107045200 |
| DOIs | |
| Publication status | Published - Jun 2013 |
| Externally published | Yes |
Publication series
| Name | Proceedings of the International Astronomical Union |
|---|---|
| Number | S299 |
| Volume | 8 |
| ISSN (Print) | 1743-9213 |
| ISSN (Electronic) | 1743-9221 |
UN SDGs
This output contributes to the following UN Sustainable Development Goals (SDGs)
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SDG 3 Good Health and Well-being
Keywords
- Coronae
- Individual (WASP-12, HD 189733)
- Magnetic fields
- Planetary systems
- Stars: activity
- Winds
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science
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