This paper reviews recent seismic findings from Kepler and K2 data. Using three years of short cadence Kepler (K1) data, it is possible to examine time evolution of pulsations in an unprecedented way. While K2 observations are shorter, only three months, they are important as they are finding more sdBV stars than K1 did. Most importantly, K2 is discovering more p-mode pulsators with coverage not possible to get from the ground.
Physics, Astronomy, and Materials Science
© 2018 the authors. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution-NonCommercial-NoDerivatives (BY-NC-ND 4.0) license.
Kepler & K2 observations of sdBV stars
Reed, Michael D., Andrzej S. Baran, John H. Telting, Roy H. Østensen, Christopher S. Jeffery, Joshua W. Kern, Laura Ketzer, John Crooke, and A. Slayton. "A review of seismic observations of Kepler and K2-Observed sdBV stars." Open Astronomy 27, no. 1 (2018): 157-166.