Seismology of delta Scuti stars in the Praesepe cluster. I. Ranges of unstable modes as predicted by linear analysis versus observations
We consider here a representative set of delta Scuti stars observed in the Praesepe cluster, thanks to recent efforts of multi-site networks. We show that the effect of rotation on the determination of fundamental parameters {Mbol} and {Teff} cannot be neglected when modelling fast rotators as delta Scuti stars. We propose a method to take this
Michel, E. et al.
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1999