About ten per cent of 'massive'stars (those of more than 1.5 solar masses) have strong, large-
scale surface magnetic fields,–. It has been suggested that merging of main-sequence and …

Magnetic confinement of stellar winds leads to the formation of magnetospheres, which can
be sculpted into centrifugal magnetospheres (CMs) by rotational support of the corotating …

This review has two parts. The first one is devoted to the Barbier–Chalonge–Divan (BCD)
spectrophotometric system, also known as the Paris spectral classification system. Although …

Context. Some Ap stars that have a strong enough magnetic field and a sufficiently low v sini
show spectral lines resolved into their magnetically split components. Aims. We present the …

Approximately 10 per cent of massive OBA main-sequence (MS) and pre-MS stars harbour
strong, large-scale magnetic fields. At the same time, there is a dearth of magnetic stars in …

About 10 per cent of stars more massive than have strong, large-scale surface magnetic
fields and are being discussed as progenitors of highly magnetic white dwarfs and …

In this introductory chapter of the Special Issue entitled 'The Structure and Evolution of Stars',
we highlight the recent major progress made in our understanding of the physics that …

Context. The initial distribution of spin rates of massive stars is a fingerprint of their elusive
formation process. It also sets a key initial condition for stellar evolution and is thus an …

The rotational and magnetic properties of many magnetic hot stars are poorly characterized,
therefore the Magnetism in Massive Stars and Binarity and Magnetic Interactions in various …

Context. So far, stellar population studies have mainly focused on the evolution of single and
binary stars. Recent observations show that triple and higher order multiple star systems are …