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

页码：91 / 98

页数：8

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