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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 Krakˇw, Poland), R.Ostensen (Instituut voor Sterrenkunde, KU Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium), J.Telting (Nordic Optical Telescope, Rambla JosÚ Ana Fernßndez PÚrez 7, 38711 Bre˝a 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.

Instituto de Astrof├şsica e Ci├¬ncias do Espa├žo Universidade do Porto Faculdade de Ciências da Universidade de Lisboa
Funda├ž├úo para a Ci├¬ncia e a Tecnologia COMPETE 2020 PORTUGAL 2020 Uni├úo Europeia