Chromospheric Properties of T-Tauri Stars Determined from EUV Spectra
Abstract
IUE spectra of six pre-main-sequence (PMS) stars are analysed and the resultant emission measure distributions compared with that of T Tau for which a chromospheric model has been calculated. Evidence for the influence of large scale motions and/or stellar winds on the transition region and coronal emission measures is found.
- Publication:
-
IAU Colloq. 71: Activity in Red-Dwarf Stars
- Pub Date:
- 1983
- Bibcode:
- 1983ards.proc..509B