A spectroscopic study of southern (candidate) gamma Doradus stars. II. Detailed abundance analysis and fundamental parameters

@article{Bruntt2008ASS,
  title={A spectroscopic study of southern (candidate) gamma Doradus stars. II. Detailed abundance analysis and fundamental parameters},
  author={Hans Bruntt and Peter De Cat and Conny Aerts},
  journal={Astronomy and Astrophysics},
  year={2008},
  volume={478},
  pages={487-496}
}
Context. The γ Doradus stars are a recent class of variable main sequence F-type stars located on the red edge of the Cepheid instability strip. They pulsate in gravity modes, and this makes them particularly interesting for detailed asteroseismic analysis, which can provide fundamental knowledge of properties near the convective cores of intermediate-mass main sequence stars. Aims. To improve current understanding of γ Dor stars through theoretical modelling, additional constraints are needed… 

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