Massive stars are important metal factories in the Universe. They have short and energetic
lives, and many of them inevitably explode as a supernova and become a neutron star or …

Magnetism is a ubiquitous property of astrophysical plasmas, yet stellar magnetism still
remains far from being completely understood. In this review, we describe recent …

Numerous magnetic hot stars exhibit gyrosynchrotron radio emission. The source electrons
were previously thought to be accelerated to relativistic velocities in the current sheet formed …

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 …

Magnetic fields can play a major role in the dynamics of outstanding explosions associated
to violent events such as gamma-ray bursts and hypernovae, since they provide a natural …

In this paper, we present the analysis of incoherent non-thermal radio emission from a
sample of hot magnetic stars, ranging from early-B to early-A spectral type. Spanning a wide …

About 10 per cent of intermediate-and high-mass dwarf stars are observed to host a strong
large-scale magnetic field at their surface, which is thought to be of fossil field origin …

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 …

Rapidly rotating early-type stars with strong magnetic fields frequently show H α emission
originating in centrifugal magnetospheres (CMs), circumstellar structures in which …

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 …