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 …

We present the first installment of a massive spectroscopic survey of Galactic O stars, based
on new, high signal-to-noise ratio, R∼ 2500 digital observations from both hemispheres …

Building on results from the Magnetism in Massive Stars (MiMeS) project, this paper shows
how a two-parameter classification of massive-star magnetospheres in terms of the magnetic …

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 …

Context. The lack of high-precision long-term continuous photometric data for large samples
of stars has impeded the large-scale exploration of pulsational variability in the OB star …

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 …

Context. The evolution of massive stars is still partly unconstrained. Mass, metallicity, mass
loss, and rotation are the main drivers of stellar evolution. Binarity and the magnetic field …

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 existence of stable magnetic configurations in white dwarfs, neutron stars, and various
non-convective stellar regions is now well recognized. It has recently been shown …