Exoplanet magnetic fields (Vidotto+, 2011)

Details Exoplanet magnetic fields (Vidotto+, 2011) Exoplanet magnetic fields (Vidotto+, 2011)

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..74119046v&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/411/L46. Originally published in: 2011MNRAS.411L..46V

Computer Science

Stars: Double And Multiple, Planets, Magnetic Fields

Scientific paper

An asymmetry between the ingress and egress times was observed in the near-UV light curve of the transit planet WASP-12b. Such asymmetry led us to suggest that the early ingress in the UV light curve of WASP-12b, compared to the optical observations, is caused by a shock around the planet, and that shocks should be a common feature in transiting systems. Here, we classify all the transiting systems known to date according to their potential for producing shocks that could cause observable light curve asymmetries.
(1 data file).

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