Frequency Regularities in δ Scuti Stars

被引：0
|
作者：
Paparo, M. [1 ]
Benko, J. M. [1 ]
机构：
[1] MTA CSFK, Konkoly Observ, Konkoly Thege Ut 15-17, H-1121 Budapest, Hungary
来源：
PROGRESS IN PHYSICS OF THE SUN AND STARS: A NEW ERA IN HELIO- AND ASTEROSEISMOLOGY | 2013年 / 479卷
关键词：
PHOTOMETRY; SATELLITE; AMPLITUDE; SPACINGS; MODES;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Space missions have produced an incredibly large database on pulsating stars. The light curves via the frequency content contain a detailed description of each star. The critical point is the identification of modes, especially in the non-asymptotic regime. The best derived parameters from the frequency content of a pulsating star light curve are the frequency differences and ratios. This presentation focuses on the potential of period ratios in mode identification.
引用
收藏
页码：91 / 98
页数：8
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