Asteroseismology of the β Cephei star KP Per

Details Asteroseismology of the β Cephei star KP Per Asteroseismology of the β Cephei star KP Per

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007coast.150..197s&link_type=abstract

Communications in Astroseismology, Vol. 150, p.197

Astronomy and Astrophysics

Astronomy

Scientific paper

We investigated the oscillations of the β 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.

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