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arXiv 2609.30881astro-ph.SRastro-ph.IM

脉动恒星中的拍频与耦合:统一的傅里叶描述与观测诊断

Beating and coupling in pulsating stars: A unified Fourier description and observational diagnostics

József M. Benkő, Emese Plachy

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中文总结 AI 辅助

该研究提出统一的傅里叶分析框架,区分脉动恒星中的调制与拍频/耦合机制,并开发诊断工具freqdiag,通过旁瓣振幅递进检验提供观测判别依据。

中文摘要 AI 辅助

脉动恒星的长期振幅和相位变化会在光变曲线傅里叶谱中,围绕脉动频率及其谐波产生旁瓣或多重结构。此类结构常被归因于调制,但线性拍频和相近振荡的非线性耦合也能产生类似模式。我们为这些替代机制发展了一个统一的分析性傅里叶描述,并识别出在其频率模式重叠时仍具判别力的观测关系。我们将信号表示为一个主导的非正弦振荡加上一个或多个与之相近的次级振荡,并解析推导出由线性叠加、二次及一般非线性耦合产生的频率、复振幅和相位。我们还利用人工光变曲线对计算现象进行了说明。我们将所得检验实现于诊断工具“freqdiag”中,该工具使用相同的归一化复振幅,将调制模型与锚定于较高或较低频率旁瓣的主-次二次耦合模型进行比较,并以旁瓣振幅递进的层次检验补充拟合。在线性拍频情形下,正弦次级信号仅产生一个额外峰值,而非正弦次级信号则产生一个谐波序列,其与主谐波的间隔随阶数增加而增大。二次耦合产生项$nf_0+lf_B$,但其振幅和相位遵循移谐和组合关系。在一般非线性阶下,耦合和调制占据相同的频率网格。该形式体系为解释类似Blazhko的RRc星、HADS变星以及其他调制与耦合难以在观测上区分的脉动恒星提供了实用框架。

英文摘要

Long-term amplitude and phase variations in pulsating stars produce side peaks or multiplets in the Fourier spectrum of the light curves around the pulsation frequency and its harmonics. Such structures are often attributed to modulation, although linear beating and the non-linear coupling of close oscillations can also produce similar patterns. We develop a unified analytical Fourier description of these alternatives and identify observational relations that retain discriminatory power when their frequency patterns overlap. We represent the signal as a dominant, non-sinusoidal oscillation plus one or more secondary oscillations close to it, and analytically derive the frequencies, complex amplitudes, and phases resulting from linear superposition, quadratic and general non-linear coupling. We also illustrate the calculated phenomena using artificial light curves. We implement the resulting tests in a diagnostic tool "freqdiag", which compares modulation with primary--secondary quadratic coupling models anchored to either the higher- or lower-frequency side peak, using the same normalized complex amplitudes, and supplements the fit with hierarchical tests of side-peak amplitude progression. A sinusoidal secondary signal produces only one additional peak in the linear-beating case, whereas a non-sinusoidal secondary signal produces a harmonic sequence, whose separation from the primary harmonics increases with order. Quadratic coupling produces terms $nf_0+lf_B$, but their amplitudes and phases follow shifted-harmonic and combination relations. At general non-linear order, coupling and modulation occupy the same frequency grid. The formalism provides a practical framework for interpreting Blazhko-like RRc stars, HADS variables, and other pulsating stars in which modulation and coupling are difficult to separate observationally.

发表机构

  • Konkoly Observatory, HUN-REN Research Centre for Astronomy and Earth Sciences(孔科利天文台,匈牙利研究与创新网络天文学与地球科学研究中心)

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