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A study of correlation between the oscillation amplitude and stellar parameters for delta Scuti stars in open clusters. Toward selection rules for delta Scuti stars oscillations

机译:振荡幅度与恒星的相关性研究   开放星团中delta scuti星的参数。走向选择规则   delta scuti恒星振荡

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摘要

In the present work, we study correlations between stellar fundamentalparameters and the oscillation amplitude for delta Scuti stars. We present thisstudy for a sample of 17 selected delta Scuti stars belonging to 5 young openclusters. Taking advantage of properties of delta Scuti stars in clusters, wecorrect the photometric parameters of our objects for the effect of fastrotation. We confirm the benefit of applying such corrections in this kind ofstudies. In addition, the technique used for this correction allows us toobtain an estimation of stellar parameters like the angle of inclination andthe rotation rate, usually not accessible. A significant correlation betweenthe parameter i' (estimation of the angle of inclination of the star) and theoscillation amplitude is found. A discussion and interpretation of these apriori surprising results is proposed, in terms of a possible selection rulefor oscillation modes of delta Scuti stars.
机译:在目前的工作中,我们研究了恒星基本参数与三角Scuti星振荡振幅之间的相关性。我们提供本研究的样本,这些样本来自5个年轻的开放性团簇中的17个选定的Scuti三角星。利用星团中Scuti星的特性,我们校正了物体的光度学参数,以实现快速旋转的效果。我们确认在此类研究中应用此类更正的好处。另外,用于此校正的技术使我们能够获得恒星参数的估计值,例如倾斜角和旋转速度,通常是无法获得的。发现参数i'(恒星倾斜角的估计值)与振荡幅度之间存在显着的相关性。提出了关于这些先验令人惊讶的结果的讨论和解释,涉及的是三角Scuti星振荡模式的可能选择规则。

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