activity
20242026
collaborators

6 papers

astro-ph.SR2026

Dust cloud lifetimes of Scallop-shell stars

Simon Daley-Yates, Moira M. Jardine, Luke Bouma

We investigate the survival of dust trapped in magnetically confined cool gas clouds (or {\it prominences}) around rapidly rotating M-dwarfs exhibiting the ``scallop-shell'' light-…

astro-ph.SR2026

Electron Cyclotron Maser Emission from Ejected Stellar Prominences on V374 Peg

C. E. Brasseur, M. M. Jardine, S. Daley-Yates +2

We investigate a possible origin for bursty radio emission observed on the active M dwarf V374 Peg, combining data-driven magnetic field modelling with archival radio light curves.…

astro-ph.EP2025

WASP-12, shrouded in mystery or just cold gas?

Simon Daley-Yates, Ricarda Beckmann, Lewis McCallum +2

Observations of the planet-hosting star WASP-12 show a distinctive depression in the \ion{Mg}{ii} and \ion{Ca}{ii} resonance lines. This has been interpreted as a marker of atmosph…

astro-ph.SR2025

Filament Mass Losses Forced by Magnetic Reconnection in the Solar Corona

Craig D. Johnston, Lars K. S. Daldorff, Peter W. Schuck +4

Recent observations of the solar atmosphere in cool extreme ultraviolet (EUV) lines have reported the prevalence of coronal rain falling from coronal cloud filaments that are assoc…

astro-ph.EP2024

Radio Signatures of Star-Planet Interactions, Exoplanets, and Space Weather

J. R. Callingham, B. J. S. Pope, R. D. Kavanagh +22

Radio detections of stellar systems provide a window onto stellar magnetic activity and the space weather conditions of extrasolar planets, information that is difficult to attain…

astro-ph.SR2024

Simulating stellar coronal rain and slingshot prominences

Simon Daley-Yates, Moira Jardine

We have numerically demonstrated that simulated cool star coronae naturally form condensations. If the star rotates slowly, with a co-rotation radius greater than the Alfvén radiu…