Mode identification of multi-periodic Slowly Pulsating B-stars: results and problems
SourceCommunications in Asteroseismology, 150, (2007), pp. 189-190
Article / Letter to editor
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Communications in Asteroseismology
We report results from mode identifications (MI) for four selected multi-periodic Slowly Pulsating B-stars (SPB) using the Fourier parameter fit (FPF) method. Problems related to the pulsational nature of these objects which hamper a correct identification are discussed. For a present day status of knowledge about SPB stars we refer to De Cat (2007, this issue).
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