  IAU Commission 35 consists of members of the International Astronomical Union
whose research is concerned with the structure and evolution of stars in all
parts of the H-R diagram. Their interests range from various aspects of stellar
interior physics, such as convection, diffusion, rotation, magnetic fields, to
asteroseismology and the prediction of the evolutionary and nucleosynthetic
histories of stars that are of vital importance for our understanding of
stellar populations and galactic chemical evolution. This report presents some
highlights that were published during the present triennial term and which
concern the field of Stellar Constitution.
