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
收藏
页码：381 / 382
页数：2
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