We are entering a golden era for stellar physics driven by satellite and telescope
observations of unprecedented quality and scope. New insights on stellar evolution and …

The age of an individual star cannot be measured, only estimated through mostly model-
dependent or empirical methods, and no single method works well for a broad range of …

With the success of the Kepler and CoRoT missions, the number of stars with detected solar-
like oscillations has increased by several orders of magnitude; for the first time we are able …

We have measured solar-like oscillations in red giants using time-series photometry from the
first 34 days of science operations of the Kepler Mission. The light curves, obtained with 30 …

We have studied solar-like oscillations in∼ 800 red giant stars using Kepler long-cadence
photometry. The sample includes stars ranging in evolution from the lower part of the red …

Context. In the context of the space missions CoRoT, Kepler, Gaia, TESS, and PLATO,
precise and accurate stellar ages, masses, and radii are of paramount importance. For …

The seismic study of the Sun and other stars offers a unique window into the interior of these
stars. Thanks to helioseismology, we know the structure of the Sun to admirable precision. In …

We studied solar-like oscillations in 115 red giants in the three open clusters, NGC 6791,
NGC 6811, and NGC 6819, based on photometric data covering more than 19 months with …

ABSTRACT NASA's Kepler mission is providing basic asteroseismic data for hundreds of
stars. One of the more common ways of determining stellar characteristics from these data is …

The Sun provides a critical benchmark for the general study of stellar structure and
evolution. Also, knowledge about the internal properties of the Sun is important for the …