activity
20002026
most citedThe surprising magnetic topology of tauSco: fossil remnant or dynamo output?

496 citations · 8.3k across the 124 of their papers we have counts for

collaborators

124 papers

astro-ph.IM2026

HRMOS: A High-Resolution Multi-Object Spectrograph for the VLT

Laura Magrini, Thomas Bensby, Sofia Randich +174

This White Paper presents the scientific rationale and instrument concept for HRMOS (High-Resolution Multi-Object Spectrograph), a next-generation instrument proposed for the ESO V…

astro-ph.SR2026

Corotating Interaction Regions (CIRs): evolution over a solar lifetime

Rose F. P. Waugh, Moira Jardine

Corotating Interaction Regions (CIRs) are persistent structures in stellar winds that arise from the interaction between fast and slow wind streams. They are known to generate shoc…

astro-ph.SR2025

Corotating Interaction Regions (CIRs): impacts with exoplanets

Rose Waugh, Moira Jardine

Corotating interaction regions (CIRs) are compressions that form in stellar winds when streams of different speeds collide. They form an Archimedean spiral around the star and can…

astro-ph.SR2025

The magnetic and spin-down properties of slowly rotating fully convective M dwarfs

Victor See, Louis Amard, Stefano Bellotti +19

The evolution of the magnetism, winds and rotation of low-mass stars are all linked. One of the most common ways to probe the magnetic properties of low-mass stars is with the Zeem…

astro-ph.SR2022★ 4 cited

Influence of magnetic cycles on stellar prominences and their mass loss rates

Sarah J. Faller, Moira M. Jardine

Observations of rapidly-rotating cool stars often show coronal slingshot prominences that remove mass and angular momentum when they are ejected. The derived masses of these promin…

astro-ph.SR2022★ 21 cited

Radio masers on WX UMa: hints of a Neptune-sized planet, or magnetospheric reconnection?

Robert D. Kavanagh, Aline A. Vidotto, Harish K. Vedantham +3

The nearby M dwarf WX UMa has recently been detected at radio wavelengths with LOFAR. The combination of its observed brightness temperature and circular polarisation fraction sugg…