24 citations · 81 across the 15 of their papers we have counts for
9 papers · 1 filter
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-…
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.…
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…
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 radius…
Heating and cooling in stellar coronae: coronal rain on a young Sun
Simon Daley-Yates, Moira M. Jardine, Craig D. Johnston
Recent observations of rapidly-rotating cool dwarfs have revealed H line asymmetries indicative of clumps of cool, dense plasma in the stars' coronae. These clumps may be either…
3D MHD models of the centrifugal magnetosphere from a massive star with an oblique dipole field
Asif ud-Doula, Stanley P. Owocki, Christopher Russell +2
We present results from new self-consistent 3D MHD simulations of the magnetospheres from massive stars with a dipole magnetic axis that has a non-zero obliquity angle () to the…
3D MHD simulations and synthetic radio emission from an oblique rotating magnetic massive star
Simon Daley-Yates, Ian R. Stevens, Asif ud-Doula
We have performed 3D isothermal MHD simulation of a magnetic rotating massive star with a non-zero dipole obliquity and predicted the radio/sub-mm observable lightcurves and contin…
Winds of Massive Magnetic Stars: Interacting Fields and Flow
Simon Daley-Yates, Ian Stevens
We present results of 3D numerical simulations of magnetically confined, radiatively driven stellar winds of massive stars, conducted using the astrophysical MHD code Pluto, with a…
Sub-mm free-free emission from the winds of massive stars in the age of ALMA
S. Daley-Yates, I. R. Stevens, T. D. Crossland
The thermal radio and sub-mm emission from the winds of massive stars is investigated and the contribution to the emission due to the stellar wind acceleration region and clumping…