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Asteroseismology of δ Scuti stars in open clusters: Praesepe

机译:疏散星团中δScuti星的星震学:Praesepe

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The present paper provides a general overview of the asteroseismic potential of delta Scuti stars in clusters, in particular focusing on convection diagnostics. We give a summarise of the last results obtained by the authors for the Praesepe cluster of which five delta Scuti stars are analysed. In that work, linear analysis is confronted with observations, using refined descriptions for the effects of rotation on the determination of the global stellar parameters and on the adiabatic oscillation frequency computations. A single, complete, and coherent solution for all the selected stars is found, which lead the authors to find important restrictions to the convection description for a certain range of effective temperatures. Furthermore, the method used allowed to give an estimate of the global parameters of the selected stars and constrain the cluster.
机译:本文提供了对星团中Scuti星的星震潜力的总体概述,尤其是对流诊断。我们总结了作者对Praesepe星团获得的最后结果,其中分析了五颗δScuti星。在这项工作中,线性分析面临着观察,对旋转对整体恒星参数的确定以及绝热振荡频率计算的影响使用了精确的描述。找到了所有选定恒星的单一,完整且一致的解,这使作者发现了在一定有效温度范围内对流描述的重要限制。此外,所使用的方法允许对选定恒星的整体参数进行估计并约束星团。

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