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 …

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 …

Aims. The composition of planetary solids and gases is largely rooted in the processing of
volatile elements in protoplanetary disks. To shed light on the key processes, we carry out a …

Many stars evolve into magnetic white dwarfs (MWDs), and observations may help to
understand when the magnetic field appears at the stellar surface, if and how it evolves …

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 …

Context. One clear manifestation of dynamo action on the Sun is the 22-yr magnetic cycle,
exhibiting a polarity reversal and a periodic conversion between poloidal and toroidal fields …

When you think about how far and fast computer science has progressed in recent years, it's
not hard to conclude that a seven-year old handbook may fall a little short of the kind of …

There is a large change in surface rotation rates of sun-like stars on the pre-main sequence
and early main sequence. Since these stars have dynamo-driven magnetic fields, this …

We describe our latest Magnetic Doppler Imaging (MDI) code capable of simultaneously
reconstructing the magnetic field vector and chemical composition distribution over the …

We report first results on a method aimed at simultaneously characterizing atmospheric
parameters and magnetic properties of M dwarfs from high-resolution near-IR spectra …