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 …

Coronal loops are the building blocks of the X-ray bright solar corona. They owe their
brightness to the dense confined plasma, and this review focuses on loops mostly as …

We present a sample of 824 solar and late-type stars with X-ray luminosities and rotation
periods. This is used to study the relationship between rotation and stellar activity and derive …

We present the results of a new study on the relationship between coronal X-ray emission
and stellar rotation in late-type main-sequence stars. We have selected a sample of 259 …

Aims. We aim to describe the pre-main-sequence and main-sequence evolution of X-ray
and extreme-ultaviolet radiation of a solar-mass star based on its rotational evolution starting …

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 …

We investigate how the observed large-scale surface magnetic fields of low-mass stars (∼
0.1–2 M⊙), reconstructed through Zeeman–Doppler imaging, vary with age t, rotation and X …

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 …

We present the discovery and validation of a three-planet system orbiting the nearby (31.1
pc) M2 dwarf star TOI-700 (TIC 150428135). TOI-700 lies in the TESS continuous viewing …

Coherent radio bursts detected from M dwarfs have some analogy with solar radio bursts but
reach orders of magnitude higher luminosities. These events trace particle acceleration …