Until the last few decades, investigations of stellar interiors had been restricted to theoretical
studies only constrained by observations of their global properties and external …

During most of their life, stars fuse hydrogen into helium in their cores. The mixing of
chemical elements in the radiative envelope of stars with a convective core is able to …

Solar gravity modes (or g modes)—oscillations of the solar interior on which buoyancy acts
as the restoring force—have the potential to provide unprecedented inference on the …

Motivated by recent interest in the phenomenon of waves transport in massive stars, we
examine whether the heat-driven gravity (g) modes excited in slowly pulsating B (SPB) stars …

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 …

Thus far, KIC 7760680 is the richest slowly pulsating B star, exhibiting 36 consecutive dipole
(ℓ= 1) gravity (g-) modes. The monotonically decreasing period spacing of the series, in …

Context. While rotation has a major impact on stellar structure and evolution, its effects are
not well understood. Thanks to high-quality and long-time base photometric observations …

Surface magnetic fields have a strong impact on stellar mass loss and rotation and, as a
consequence, on the evolution of massive stars. In this work, we study the influence of an …

The large-scale magnetic fields detected at the surface of about 10% of hot stars extend into
the stellar interior, where they may alter the structure. Deep inner regions of stars are only …

Context. The discovery of moderate differential rotation between the core and the envelope
of evolved solar-like stars could be the signature of a strong magnetic field trapped inside …