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 …

Stars lose a significant amount of angular momentum between birth and death, implying that
efficient processes transporting it from the core to the surface are active. Space …

The angular momentum (AM) evolution of stellar interiors, along with the resulting rotation
rates of stellar remnants, remains poorly understood. Asteroseismic measurements of red …

The determination of exoplanet properties and occurrence rates using Kepler data critically
depends on our knowledge of the fundamental properties (such as temperature, radius, 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 …

We present 3D simulations of the core-collapse of massive rotating and non-rotating
progenitors performed with the general relativistic neutrino hydrodynamics code coconut …

Kepler ultra-high precision photometry of long and continuous observations provides a
unique dataset in which surface rotation and variability can be studied for thousands of stars …

A red giant star is an evolved low-or intermediate-mass star that has exhausted its central
hydrogen content, leaving a helium core and a hydrogen-burning shell. Oscillations of stars …

The angular momentum (AM) content of massive stellar cores helps us to determine the
natal spin rates of neutron stars and black holes. Asteroseismic measurements of low-mass …

Abstract The Rossiter–McLaughlin effect observed for transiting exoplanets often requires
prior knowledge of the stellar projected equatorial rotational velocity (v sin i). This is usually …