Variability of M giant stars based on Kepler photometry: general characteristics

被引：0

作者：

Banyai, E. ^{[1
]}

Kiss, L. L. ^{[1
]}

机构：

[1] Hungarian Acad Sci, Konkoly Observ, Konkoly Thege M Ut 15-17, H-1121 Budapest, Hungary

来源：

PRECISION ASTEROSEISMOLOGY | 2014年 / 9卷 / 301期

关键词：

stars: variables: other; stars: AGB and post-AGB; techniques: photometric;

D O I：

10.1017/S1743921313014658

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Our study based on the continuous, high-precision observations covering more than three years provided by the Kepler mission reveals a new systematic effect in the data, a possible transition region between solar-like and Mira-like oscillations, and gives an overview of M giant variability on a wide range of time-scales (hours to years).

引用

页码：381 / 382

页数：2

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