Aims.We investigate theoretical pulsation models for the δ Scuti star 44 Tau. The star was monitored during several multisite campaigns which confirmed the presence of radial and nonradial oscillations. Its exceptionally low rotational velocity makes 44 Tau particulary interesting for an asteroseismic study. Due to the measured log g value of 3.6 ± 0.1, main sequence and post-main sequence models have to be considered.
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Lenz et al. (2007) studied this question.
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