Saesen, S. ; Briquet, M. ; Cuypers, J. ; De Cat, P. ; Goossens, K.

published in Communications in Asteroseismology, 150, pp. 197 (2007)

Abstract: We investigated the oscillations of the ß Cephei star KP Per (HD 21803, B2IV, V=6.41) using Geneva photometry. We performed a detailed frequency analysis and a mode identification by means of photometric amplitude ratios. Then we confronted our deduced observational oscillation spectrum with that predicted by theory in order to determine a range for some stellar parameters, such as the mass and radius of KP Per.

DOI: 10.1553/cia150s197
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