Variability of M giant stars based on Kepler photometry: general characteristics
Abstract
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).
- Publication:
-
Precision Asteroseismology
- Pub Date:
- February 2014
- DOI:
- 10.1017/S1743921313014658
- arXiv:
- arXiv:1405.1624
- Bibcode:
- 2014IAUS..301..381B
- Keywords:
-
- stars: variables: other;
- stars: AGB and post-AGB;
- techniques: photometric;
- Astrophysics - Solar and Stellar Astrophysics
- E-Print:
- 3 pages, 1 figures, conference proceeding