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

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...

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Bibliographic Details
Published inProceedings of the International Astronomical Union Vol. 9; no. S301; pp. 381 - 382
Main Authors Bányai, E., Kiss, L. L.
Format Journal Article
LanguageEnglish
Published Cambridge, UK Cambridge University Press 01.08.2013
Subjects
Astronomy
Astrophysics
Contributed Papers
Giant stars
stars: AGB and post-AGB
techniques: photometric
stars: variables: other
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Summary: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).
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ISSN:1743-9213
1743-9221
DOI:10.1017/S1743921313014658