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

Context. The Gaia mission has delivered hundreds of thousands of variable star light curves
in multiple wavelengths. Recent work demonstrates that these light curves can be used to …

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 …

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 …

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 …

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 …

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

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 …

Magnetic B-stars often exhibit circularly polarized radio emission thought to arise from
gyrosynchrotron emission by energetic electrons trapped in the circumstellar …