52 citations · 52 across the 4 of their papers we have counts for
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Stellar mass ejections
M. Jardine, J. -F. Donati, S. G. Gregory
It has been known for some time now that rapidly-rotating solar-like stars possess the stellar equivalent of solar prominences. These may be three orders of magnitude more massive…
Modeling X-ray emission from stellar coronae
S. G. Gregory, M. Jardine, C. Argiroffi +1
By extrapolating from observationally derived surface magnetograms of low-mass stars we construct models of their coronal magnetic fields and compare the 3D field geometry with axi…
Why are accreting T Tauri stars less luminous in X-rays than non-accretors?
S. G. Gregory, K. Wood, M. Jardine
Accreting T Tauri stars are observed to be less luminous in X-rays than non-accretors, an effect that has been detected in various star forming regions. To explain this we have com…
Why are accreting T Tauri stars observed to be less luminous in X-rays than non-accretors?
S. G. Gregory, K. Wood, M. Jardine
Accreting T Tauri stars are observed to be less luminous in X-rays than non-accretors, an effect that has been detected in various star forming regions. To explain this we have com…