快速旋转和声学模式

Q3 Multidisciplinary

Bulletin de la Societe Royale des Sciences de Liege Pub Date : 2020-01-14 DOI:10.25518/0037-9565.9276

D. Reese

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引用次数: 0

摘要

在这篇文章中，我们描述了在快速旋转恒星声脉动建模方面的最新进展。然后，我们继续描述最近在解释两颗观测到的恒星的脉动光谱方面的尝试。这些利用多色模式可见性，模式激发和脉动频率，以限制观察模式的识别。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

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Fast rotation and acoustic modes

In this contribution, we describe recent progress in modelling acoustic pulsations of rapidly rotating stars. We then go on to describe very recent attempts at interpreting pulsation spectra in two observed stars. These make use of multi-colour mode visibilities, mode excitation, and pulsation frequencies in order to con-strain the identification of the observed modes.

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来源期刊

Bulletin de la Societe Royale des Sciences de Liege Multidisciplinary-Multidisciplinary

CiteScore

0.90

自引率

0.00%

发文量

期刊介绍： The ‘Société Royale des Sciences de Liège" (hereafter the Society) regularly publishes in its ‘Bulletin" original scientific papers in the fields of astrophysics, biochemistry, biophysics, biology, chemistry, geology, mathematics, mineralogy or physics, following peer review approval.