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Variability of M giant stars based on Kepler photometry: general characteristics
Published online by Cambridge University Press: 18 February 2014
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).
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 9 , Symposium S301: Precision Asteroseismology , August 2013 , pp. 381 - 382
- Copyright
- Copyright © International Astronomical Union 2014
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