▪ Abstract In this article we first review the main physical effects to be considered in the
building of evolutionary models of rotating stars on the Upper Main-Sequence (MS). The …

Oscillations detected on the solar surface provide a unique opportunity for investigations of
the interior properties of a star. Through major observational efforts, including extensive …

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 …

Context. The chemical composition of the Sun is a fundamental yardstick in astronomy,
relative to which essentially all cosmic objects are referenced. As such, having accurate …

Data from the Global Oscillation Network Group (GONG) project and other helioseismic
experiments provide a test for models of stellar interiors and for the thermodynamic and …

We propose a simple interpretation of the rotation period data for solar-and late-type stars.
The open cluster and Mount Wilson star observations suggest that rotating stars lie primarily …

The splitting of the frequencies of the global resonant acoustic modes of the Sun by large-
scale flows and rotation permits study of the variation of angular velocity Ω with both radius …

Grids of models for rotating stars are constructed in the range of 9 to 120 M $ _ {\odot} $ at
solar metallicity. The following effects of rotation are included: shellular rotation, new …

Evolution of Stars and Stellar Populations is a comprehensive presentation of the theory of
stellar evolution and its application to the study of stellar populations in galaxies. Taking a …

Helium and heavy-element diffusion are both included in precise calculations of solar
models. In addition, improvements in the input data for solar interior models are described …