52 citations · 53 across the 2 of their papers we have counts for
2 papers
astro-ph.SR2009★ 1 cited
Multi-wavelength observing of a forming solar-like star
S. G. Gregory, E. Flaccomio, C. Argiroffi +7
V2129 Oph is a 1.35 solar mass classical T Tauri star, known to possess a strong and complex magnetic field. By extrapolating from an observationally derived magnetic surface map,…
astro-ph2007★ 52 cited
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…