Observations of pulsations in roAp stars

Third Coast Pub Date : 2007-02-09 DOI:10.1553/cia150s39
O. Kochukhov
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引用次数: 262

Abstract

I review recent results of the observations of magnetoacoustic p-mode oscillations in roAp stars with the focus on time-resolved spectroscopic studies. Time-series spectroscopy of roAp stars reveals unexpected and diverse pulsational behaviour in the spectral lines of different chemical elements. These unique pulsational characteristics arise from an interplay between the short vertical length of pulsation waves and extreme chemical stratification in the atmospheres of peculiar stars. This enables a tomographic reconstruction of the depth-dependence of the chemical composition and pulsation wave properties. The combination of magnetoacoustic tomography with Doppler imaging of the horizontal non-radial pulsation pattern opens the possibility for an unprecedented three-dimensional mapping of roAp star atmospheres.
恒星脉动的观测
本文综述了近年来对roAp恒星的磁声p模振荡的观测结果,重点是时间分辨光谱研究。roAp恒星的时间序列光谱揭示了不同化学元素谱线中意想不到的不同脉动行为。这些独特的脉动特征来自于脉动波的短垂直长度和特殊恒星大气中极端的化学分层之间的相互作用。这使得层析重建的深度依赖的化学成分和脉冲波的性质。磁声层析成像与水平非径向脉动模式的多普勒成像相结合,为前所未有的roAp恒星大气三维测绘提供了可能。
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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