BRITE view of $\ddot{I}ƒ$ Scorpii, ${\hat{I}}^2$ Cephei-type star studied for over a century

Abstract

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.

3 pages, 1 figure, to appear in the Proceedings of the 3rd BRITE Science Conference, Auberge du Lac Taureau, Canada