Long-term variability of T Tauri stars using WASP
Long-term variability of T Tauri stars using WASP
We present a reference study of the long-term optical variability of young stars using data from the WASP project. Our primary sample is a group of well-studied classical T Tauri stars (CTTSs), mostly in Taurus–Auriga. WASP light curves cover time-scales of up to 7 yr and typically contain 10 000–30 …