Yearslong time series of high-precision brightness measurements have been assembled for
thousands of stars with telescopes operating in space. Such data have allowed astronomers …

Stars lose a significant amount of angular momentum between birth and death, implying that
efficient processes transporting it from the core to the surface are active. Space …

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 …

Magnetars are highly magnetized neutron stars, the formation mechanism of which is
unknown. Hot helium-rich stars with spectra dominated by emission lines are known as Wolf …

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 …

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 …

The magnetic white dwarfs (MWDs) are found either isolated or in interacting binaries. The
isolated MWDs divide into two groups: a high field group (10 5–10 9 G) comprising some …

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 …

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 …

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 …