Red-giant seismic properties analyzed with CoRoT

@article{Mosser2010RedgiantSP,
  title={Red-giant seismic properties analyzed with CoRoT},
  author={Beno{\^i}t Mosser and K'evin Belkacem and M-J. Goupil and Andrea Miglio and Thierry Morel and Caroline Barban and Frédéric Baudin and Saskia Hekker and R'eza Samadi and Joris De Ridder and Werner W. Weiss and Michel Auvergne and Annie Baglin},
  journal={Astronomy and Astrophysics},
  year={2010},
  volume={517},
  pages={1-11}
}
Context. The CoRoT 5-month long observation runs provide us with the opportunity to analyze a large variety of red-giant stars and derive their fundamental parameters from their asteroseismic properties. Aims. We perform an analysis of more than 4600 CoRoT light curves to extract as much information as possible. We take into account the characteristics of both the star sample and the method to ensure that our asteroseismic results are as unbiased as possible. We also study and compare the… 
Mixed modes in red-giant stars observed with CoRoT
Context. The CoRoT mission has provided thousands of red-giant light curves. The analysis of their solar-like oscillations allows us to characterize their stellar properties. Aims. Up to now, the
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The CoRoT and Kepler missions provide us with thousands of red-giant light curves that allow a very precise asteroseismic study of these objects. Before CoRoT and Kepler , the red-giant oscillation
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Context. Clear power excess in a frequency range typical for solar-type oscillations in red giants has been detected in more than 1000 stars, which have been observed during the first 138 days of the
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We present the asteroseismic analysis of 1948 F-, G- and K-type main-sequence and subgiant stars observed by the National Aeronautics and Space Administration Kepler mission. We detect and
Atmospheric parameters and chemical properties of red giants in the CoRoT asteroseismology fields
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Context. The space mission Kepler provides us with long and uninterrupted photometric time series of red giants. This allows us to examine their seismic global properties and to compare these with
Differential asteroseismic study of seismic twins observed by CoRoT - Comparison of HD 175272 with HD 181420
Context. The CoRoT short asteroseismic runs give us the opportunity to observe a large variety of late-type stars through their solarlike oscillations. We report the observation and modeling of the
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The clear detection with CoRoT and KEPLER of radial and non-radial solar-like oscillations in many red giants paves the way for seismic inferences on the structure of such stars. We present an
Solar-like oscillations in red giants observed with Kepler: comparison of global oscillation parameters from different methods
Context. The large number of stars for which uninterrupted high-precision photometric timeseries data are being collected with Kepler and CoRoT initiated the development of automated methods to
The CoRoT‐GES Collaboration: Improving red giants spectroscopic surface gravitity and abundances with asteroseismology
Nowadays large spectroscopic surveys, like the Gaia-ESO Survey (GES), provide unique stellar databases for better investigating the formation and evolution of our Galaxy. Great attention must be paid
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