Poster abstract details
Seismic analysis and interpretation of multi-month long Kepler time series of Sun-like stars
Abstract
Since the launch of the Kepler satellite, a few Sun-like stars
have been observed at least for the first 7 months of science operations
at high cadence. We selected four of these stars whose magnitudes are
in the range from 10.5 to 12 and whose effective temperatures span the
interval between 5200 and 6300 K, according to the Kepler Input
Catalogue. We present the results obtained from the extraction of global
seismic parameters as well as a detailed frequency analysis and
interpretation based on dedicated peak-bagging of these stars.
have been observed at least for the first 7 months of science operations
at high cadence. We selected four of these stars whose magnitudes are
in the range from 10.5 to 12 and whose effective temperatures span the
interval between 5200 and 6300 K, according to the Kepler Input
Catalogue. We present the results obtained from the extraction of global
seismic parameters as well as a detailed frequency analysis and
interpretation based on dedicated peak-bagging of these stars.