Abstract
The Kepler spacecraft is providing photometric time series with micro-magnitude precision for thousands of variable stars, what opens up opportunities to study the pulsational variability in much more detail than was previously possible from the ground. We present a first general characterization of the variability of A-F type stars as observed in the Kepler light curves of a sample of 750 candidate A-F type stars.
Cite
CITATION STYLE
APA
Uytterhoeven, K. (2013). The new kepler picture of variability among a and f type stars. In Astrophysics and Space Science Proceedings (Vol. 31, pp. 231–235). Springer Netherlands. https://doi.org/10.1007/978-3-642-29630-7_43
Register to see more suggestions
Mendeley helps you to discover research relevant for your work.
Already have an account? Sign in
Sign up for free