We review the application of the one-dimensional Mixing Length Theory (MLT) model of
convection in stellar interiors and low-mass stellar evolution. We summarize the history of …

The convective envelopes of solar-type stars and the convective cores of intermediate-and
high-mass stars share boundaries with stable radiative zones. Through a host of processes …

Context. The multiplicity fraction of stars, down to the substellar regime, is a parameter of
fundamental importance for stellar formation, evolution, and planetology. The census of …

Stellar physics and evolution calculations enable a broad range of research in astrophysics.
Modules for Experiments in Stellar Astrophysics (MESA) is a suite of open source, robust …

We use asteroseismic data from the Kepler satellite to determine fundamental stellar
properties of the 66 main-sequence targets observed for at least one full year by the mission …

Context. In the era of large Galactic stellar surveys, carefully calibrating and validating the
data sets has become an important and integral part of the data analysis. Moreover, new …

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 …

Context. Rotational splittings are currently measured for several main sequence stars and a
large number of red giants with the space mission Kepler. This will provide stringent …

Context. There are now more than 22 months of long-cadence data available for thousands
of red giants observed with the Kepler space mission. Consequently, we are able to clearly …

Asteroseismology of stars that exhibit solar-like oscillations are enjoying a growing interest
with the wealth of observational results obtained with the CoRoT and Kepler missions. In this …