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- W6995174 abstract "In addition, a hot Jupiter’s tidal influence on its star may increase the stellar rotation rate and thus also increase the global stellar activity level. Our recent work has shown that stars with hot Jupiters have twice the UV emission than stars with planets in wider orbits, which is also anti-correlated with the stellar synchronization time scales. Even though the stars with hot Jupiters are not fully synchronized (full synchronization in most cases will take longer than the age of the Universe), they have already undergone some increase in rotation rate, provided that the planets migrated early on in the system’s history. Studying both tidal and magnetic star-planet interactions aids our understanding of the formation, migration and evolution of hot Jupiters, and provides the best-available probe of exoplanetary magnetic fields." @default.
- W6995174 created "2016-06-24" @default.
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- W6995174 date "2010-05-01" @default.
- W6995174 modified "2023-10-18" @default.
- W6995174 title "Star-Planet Interactions: The Tidal and Magnetic Influence of Hot Jupiters" @default.
- W6995174 hasPublicationYear "2010" @default.
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