The advent of the second data release of the Gaia mission, in combination with data from
large spectroscopic surveys, is revolutionizing our understanding of the Galaxy. Thanks to …

Yearslong time series of high-precision brightness measurements have been assembled for
thousands of stars with telescopes operating in space. Such data have allowed astronomers …

To date, the radial velocity (RV) method has been one of the most productive techniques for
detecting and confirming extrasolar planetary candidates. Unfortunately, stellar activity can …

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 Kepler mission has provided exquisite data to perform an ensemble asteroseismic
analysis on evolved stars. In this work we systematically characterize solar-like oscillations …

There has been an incredibly large investment in obtaining high-resolution stellar spectra for
determining chemical abundances of stars. This information is crucial to answer …

Turbulent Rayleigh-Bénard convection displays a large-scale order in the form of rolls and
cells on lengths larger than the layer height once the fluctuations of temperature and velocity …

We use asteroseismic data obtained by the NASA Kepler mission to estimate the
fundamental properties of more than 500 main-sequence and sub-giant stars. Data obtained …

We have analyzed solar-like oscillations in∼ 1700 stars observed by the Kepler Mission,
spanning from the main sequence to the red clump. Using evolutionary models, we test …

Asteroseismology involves probing the interiors of stars and quantifying their global
properties, such as radius and age, through observations of normal modes of oscillation …