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• W127719107 abstract "Since the advent of space asteroseismology, enabled by the CoRoT and Kepler space-craft, solar-like oscillations have appeared to be a common feature of low-mass stars from the main-sequence to the red-giant phases. In this context, scaling relations that relate asteroseismological quantities and stellar parameters are an essential tool in the study a large class of stars. Most of these relations concern the connection between pulsations and turbulent convection. Therefore, a deep investigation of this connection is necessary to obtain insight into the processes underlying mode driving and damping and consequently to improve our knowledge of the scaling relations. This is a key step that will permit us to perform a leap forward in our understanding of stellar interiors." @default.
• W127719107 created "2016-06-24" @default.
• W127719107 creator A5045703915 @default.
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• W127719107 date "2013-01-01" @default.
• W127719107 modified "2023-10-11" @default.
• W127719107 title "Connections Between Stellar Oscillations and Turbulent Convection" @default.
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• W127719107 doi "https://doi.org/10.1007/978-3-642-33380-4_9" @default.
• W127719107 hasPublicationYear "2013" @default.
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