Talk abstract details

We present preliminary results for a few new pre-main-sequence candidate pulsating stars in the CoRoT fields. These objects were selected on the basis of the presence of Halpha emission in their spectra. We present the frequency spectra for the target star and
provide a possible interpretation of the detected features at the light of present knowledge. When possible we try an asteroseismic interpretation
of the data by comparison with updated radial and non-radial models.