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• W3100692371 startingPage "A124" @default.
• W3100692371 abstract "Context. The study of stellar activity is important because it can provide new constraints for dynamo models when combined with surface rotation rates and the depth of the convection zone. We know that the dynamo mechanism, which is believed to be the main process that rules the magnetic cycle of solar-like stars, results from the interaction between (differential) rotation, convection, and magnetic field. The Kepler mission has already been collecting data for a large number of stars during four years allowing us to investigate magnetic stellar cycles." @default.
• W3100692371 created "2020-11-23" @default.
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• W3100692371 date "2014-02-01" @default.
• W3100692371 modified "2023-10-11" @default.
• W3100692371 title "Magnetic activity of F stars observed by<i>Kepler</i>" @default.
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• W3100692371 doi "https://doi.org/10.1051/0004-6361/201322707" @default.
• W3100692371 hasPublicationYear "2014" @default.
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