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Seismology of the Sun and the Distant Stars 2016
Using Today’s Successes to Prepare the Future
Joint TASC2 & KASC9 Workshop – SPACEINN & HELAS8 Conference

EPIC 212707862, a pulsating subdwarf B star from Kepler K2 mission.
Szymon Bachulski (Pedagogical University of Cracow, Poland), A.Baran (The Pedagogical University of Cracow, ul. Podchorążych 2, 30-084 Kraków, Poland), R.Ostensen (Instituut voor Sterrenkunde, KU Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium), J.Telting (Nordic Optical Telescope, Rambla José Ana Fernández Pérez 7, 38711 Breña Baja, Spain), M.Reed (Department of Physics, Astronomy, and Materials Science, Missouri State University, Springfield, MO 65804, USA)

We present our analysis of Kepler K2 data of EPIC 212707862, a pulsating subdwarf B star (sdBV). We extracted 12 significant pulsation modes from nearly 79 days of continuous data gathered during Campaign 6. In the case of this star we did not find any signs of multiplets which would enable us to derive a rotation period. We also searched for period-spacing sequences to perform a mode identification, and we successfully identified modal degrees of 11 of 12 detected modes.

Faculdade de Ciências da Universidade de Lisboa Universidade do Porto Faculdade de Ciências e Tecnologia da Universidade de Coimbra
Fundação para a Ciência e a Tecnologia COMPETE 2020 PORTUGAL 2020 União Europeia