Abstract
The oblique pulsator model is introduced for the roAp stars in the case of the best-studied star, HR 3831. A detailed discussion of some techniques and pitfalls of frequency analysis is given. Developments of the oblique pulsator model from both theoretical and observational viewpoints are given and problems discussed.
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© 2000 Springer Science+Business Media Dordrecht
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Kurtz, D.W. (2000). Evidence for, and Development of, the Oblique Pulsator Model. In: İbanoğlu, C. (eds) Variable Stars as Essential Astrophysical Tools. NATO Science Series, vol 544. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4299-1_13
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DOI: https://doi.org/10.1007/978-94-011-4299-1_13
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