We present the analysis performed on spectropolarimetric data of 97 O-type targets included
in the framework of the MiMeS (Magnetism in Massive Stars) Survey. Mean Least-Squares …

Abstract The MiMeS (Magnetism in Massive Stars) project is a large-scale, high-resolution,
sensitive spectropolarimetric investigation of the magnetic properties of O-and early B-type …

Massive stars are crucial building blocks of galaxies and the universe, as production sites of
heavy elements and as stirring agents and energy providers through stellar winds 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 …

While magnetic fields have long been considered significant for the evolution of magnetic
non-degenerate stars and compact stars, it has become clear in recent years that, in fact, all …

We examine the angular momentum loss and associated rotational spin-down for magnetic
hot stars with a line-driven stellar wind and a rotation-aligned dipole magnetic field. Our …

We summarize the results of a spectropolarimetric survey of 56 chemically peculiar (CP)
stars in the association of Orion OB1. We uniformly collected the observational material with …

Aims. We test predictions of evolution models on mixing of CNO-cycled products in massive
stars from a fundamental perspective. Relative changes within the theoretical C: N: O …

The last few decades have seen significant progress in our understanding of the occurrence
of magnetic fields in stars with radiative envelopes, in particular in massive stars and in …

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 …