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Chapitre D'ouvrage Année : 2013

Connections Between Stellar Oscillations and Turbulent Convection

Résumé

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.

Dates et versions

hal-03692059 , version 1 (09-06-2022)

Identifiants

Citer

Kevin Belkacem, Davoud-Reza Samadi. Connections Between Stellar Oscillations and Turbulent Convection. Studying Stellar Rotation and Convection, Lecture Notes in Physics, 865, pp.179, 2013, ⟨10.1007/978-3-642-33380-4_9⟩. ⟨hal-03692059⟩
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