Blazhko effect in Cepheids and RR Lyrae stars

被引:2
|
作者
Szabo, Robert [1 ]
机构
[1] Hungarian Acad Sci, Konkoly Observ, Res Ctr Astron & Earth Sci, Konkoly Thege Miklos Ut 15-17, H-1121 Budapest, Hungary
来源
PRECISION ASTEROSEISMOLOGY | 2014年 / 9卷 / 301期
关键词
stars: variables: RR Lyrae; stars: variables: Cepheids; Blazhko effect; stars: individual: RR Lyr; V445; Lyr; V473; alpha UMi; pulsation; hydrodynamics; Kepler; LARGE-MAGELLANIC-CLOUD; FREQUENCY-ANALYSIS; PERIOD; PHOTOMETRY; MODE;
D O I
10.1017/S1743921313014397
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Blazhko effect is the conspicuous amplitude and phase modulation of the pulsation of RR Lyrae stars that was discovered in the early 20th century. The field of study of this mysterious modulation has recently been invigorated thanks to the space photometric missions providing long, uninterrupted, ultra-precise time-series data. In this paper I give a brief overview of the new observational findings related to the Blazhko effect, such as extreme modulations, irregular modulation cycles and additional periodicities. I argue that these findings together with dedicated ground-based efforts provide us now with a fairly complete picture and a good starting point to theoretical investigations. Indeed, new, unpredicted dynamical phenomena have been discovered in Blazhko RR Lyrae stars, such as period doubling, high-order resonances, three-mode pulsation and low-dimensional chaos. These led to the proposal of a new explanation to this century-old enigma, namely a high-order resonance between radial modes. Along these lines I present the latest efforts and advances from the theoretical point of view. Lastly, amplitude variations in Cepheids are discussed.
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页码:241 / 248
页数:8
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