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Models of red giants in the CoRoT asteroseismology fields combining asteroseismic and spectroscopic constraints

Published online by Cambridge University Press:  27 October 2016

Lagarde Nadège
Lagarde Nadège*
Affiliation:
School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK email: lagarde@bison.ph.bham.ac.uk
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Abstract

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The availability of asteroseismic constraints for a large sample of red-giant stars from the CoRoT and Kepler missions paves the way for various statistical studies of the seismic properties of stellar populations. We use a detailed spectroscopic study of 19 CoRoT red-giant stars (Morel et al. 2014) to compare theoretical stellar evolution models to observations of the open cluster NGC 6633 and field stars. This study is already published in Lagarde et al. (2015)

Keywords

asteroseismologystars: abundancesstars: evolutionstars: rotationstars: interiors
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29B: Astronomy in Focus , August 2015 , pp. 525 - 528
Copyright
Copyright © International Astronomical Union 2016 

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