How has the solar wind evolved to reach what it is today? In this review, I discuss the long-
term evolution of the solar wind, including the evolution of observed properties that are …

The Sun and other stars are magnetic: magnetism pervades their interiors and affects their
evolution in a variety of ways. In the Sun, both the fields themselves and their influence on …

BANYAN Σ is a new Bayesian algorithm to identify members of young stellar associations
within 150 pc of the Sun. It includes 27 young associations with ages in the range∼ 1–800 …

Magnetic fields play a fundamental role for interior and atmospheric properties of M dwarfs
and greatly influence terrestrial planets orbiting in the habitable zones of these low-mass …

Understanding massive stars is essential for a variety of branches of astronomy including
galaxy and star cluster evolution, nucleosynthesis and supernovae, pulsars, and black …

About ten per cent of 'massive'stars (those of more than 1.5 solar masses) have strong, large-
scale surface magnetic fields,–. It has been suggested that merging of main-sequence and …

Context. Early B-type stars are ideal indicators for present-day cosmic abundances since
they preserve their pristine abundances and typically do not migrate far beyond their birth …

Context. Understanding how star formation begins and propagates through molecular
clouds is a fundamental but still open question. One major difficulty in addressing this …

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 …

Mass loss is a key process in the evolution of massive stars, and must be understood
quantitatively if it is to be successfully included in broader astrophysical applications such as …