KEPLER TELESCOPE AND SOLAR-LIKE PULSATORS

摘要

We present 104 stars selected for a long-time monitoring for Kepler, a new NASA space telescope. 30 of these stars are primary asteroseismological targets for Kepler, the remaining 74, secondary asteroseismological targets for the telescope. They are mostly F-K stars that we expect to show solar-like oscillations. We determine fundamental astrophysical parameters and estimate pulsational properties of the selected targets. Then, we use simulations to present Kepler's ability of detection oscillations with frequencies and amplitudes typical for solar-like pulsators.