BRITE view of σ Scorpii, β Cephei-type star studied for over a century
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🌌 astro-ph.SR
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britestarmodespresentedresultsallowedanalysisbeta
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Preliminary results of the analysis of the combined space-based BRITE and SMEI, and ground-based Stroemgren photometry are presented. The BRITE data allowed to find seven p and three g modes in the frequency spectrum of this star; only four p modes were known in this star prior to this study. The first results of seismic modelling are also presented.
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