International audienceContext: T Tauri stars exhibit variability on all timescales, whose origin is still debated. On WTTS the variability is fairly simple and attributed to long-lived, ubiquitous cool spots. Aims: We investigate the long term variability of WTTS, extending up to 20 years in some cases, characterize it statistically and discuss its implications for our understanding of these stars. Methods: We have obtained a unique, homogeneous database of photometric measurements for WTTS extending up to 20 years. It contains more than 9000 UBVR observations of 48 WTTS. All the data were collected at Mount Maidanak Observatory (Uzbekistan) and they constitute the longest homogeneous record of accurate WTTS photometry ever assembled. Resul...
We present a reference study of the long-term optical variability of young stars using data from the...
Context. V1184 Tau is a young variable that for a long time has been monitored at optical wavelength...
Aims. The main purpose of our investigation is to construct the long-time light curve of the PMS st...
International audienceContext: T Tauri stars exhibit variability on all timescales, whose origin is ...
International audienceContext: T Tauri stars exhibit variability on all timescales, whose origin is ...
International audienceContext: T Tauri stars exhibit variability on all timescales, whose origin is ...
Context.T Tauri stars exhibit variability on all timescales, whose origin is still debated. ...
Context.T Tauri stars exhibit variability on all timescales, whose origin is still debated. ...
We present a unique, homogeneous database of photometric measurements for Classical T Tauri stars ex...
We present a study of the long-term optical variability of young T Tauri stars using previously unpu...
We present photometric light curves of T Tauri Stars (TTS) observed in the Southern hemisphere. Our...
We present photometric light curves of T Tauri Stars (TTS) observed in the Southern hemisphere. Our...
We present a reference study of the long-term optical variability of young stars using data from the...
We monitored the light variations of 22 weak-line T Tauri stars (WTTS) discovered among the X-ray so...
Context: .The ROSAT All-Sky Survey detected many young objects outside any known star forming region...
We present a reference study of the long-term optical variability of young stars using data from the...
Context. V1184 Tau is a young variable that for a long time has been monitored at optical wavelength...
Aims. The main purpose of our investigation is to construct the long-time light curve of the PMS st...
International audienceContext: T Tauri stars exhibit variability on all timescales, whose origin is ...
International audienceContext: T Tauri stars exhibit variability on all timescales, whose origin is ...
International audienceContext: T Tauri stars exhibit variability on all timescales, whose origin is ...
Context.T Tauri stars exhibit variability on all timescales, whose origin is still debated. ...
Context.T Tauri stars exhibit variability on all timescales, whose origin is still debated. ...
We present a unique, homogeneous database of photometric measurements for Classical T Tauri stars ex...
We present a study of the long-term optical variability of young T Tauri stars using previously unpu...
We present photometric light curves of T Tauri Stars (TTS) observed in the Southern hemisphere. Our...
We present photometric light curves of T Tauri Stars (TTS) observed in the Southern hemisphere. Our...
We present a reference study of the long-term optical variability of young stars using data from the...
We monitored the light variations of 22 weak-line T Tauri stars (WTTS) discovered among the X-ray so...
Context: .The ROSAT All-Sky Survey detected many young objects outside any known star forming region...
We present a reference study of the long-term optical variability of young stars using data from the...
Context. V1184 Tau is a young variable that for a long time has been monitored at optical wavelength...
Aims. The main purpose of our investigation is to construct the long-time light curve of the PMS st...