No CrossRef data available.
Article contents
Hα and NaD Line Variability in RY Tauri
Published online by Cambridge University Press: 12 April 2016
Abstract
Using high resolution spectroscopy of the T Tau star RY Tau in the regions of Hα and Na D lines, we discovered line profile variability, which is interpreted by a hypothesis of stellar ’prominences’: cool gas clouds are moving inside the stellar wind, ascending and descending on a time scale of a few days. These clouds are supposed to be controlled by the magnetic field of the star. The range of radial velocities of the clouds (−100 to +100 km/s) is twice as large as the rotational velocity (v sin i) of the star. The form of variability of the Hα profile suggests the existence of two components: the (variable) stellar wind and the circumstellar disc.
- Type
- Part IV Stellar activity
- Information
- Copyright
- Copyright © Springer-Verlag 1991