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 …

Cool stars like the Sun harbor convection zones capable of producing substantial surface
magnetic fields leading to stellar magnetic activity. The influence of stellar parameters like …

Coherent low-frequency (≲ 200 MHz) radio emission from stars encodes the conditions of
the outer corona, mass-ejection events and space weather,,,–. Previous low-frequency …

Observing magnetic star–planet interactions (SPIs) offers promise for determining the
magnetic fields of exoplanets. Models of sub-Alfvénic SPIs predict that terrestrial planets in …

X-ray emission from stars in the cool half of the Hertzsprung-Russell diagram is generally
attributed to the presence of a magnetic corona that contains plasma at temperatures …

Aims. We study the evolution of stellar rotation and wind properties for low-mass main-
sequence stars. Our aim is to use rotational evolution models to constrain the mass loss …

▪ Abstract Radio astronomy has provided evidence for the presence of ionized atmospheres
around almost all classes of nondegenerate stars. Magnetically confined coronae dominate …

We present the first results of the Gould's Belt Distances Survey (GOBELINS), a project
aimed at measuring the proper motion and trigonometric parallax of a large sample of young …

We have used the ASCA and ROSAT X-ray satellites to probe the coronae of a sample of
nine solar-like G stars. These stars are all ostensibly single with ages ranging from 70 Myr to …

Radiation belts are present in all large-scale Solar System planetary magnetospheres:
Earth, Jupiter, Saturn, Uranus and Neptune. These persistent equatorial zones of relativistic …