The ultraviolet spectrum of Zeta Tauri.
Abstract
Three IUE high resolution spectra of the Be star Zeta Tauri have been studied. The radial velocities of the N I components formed in the extended atmosphere show that the shell is now quiescent. The far ultraviolet spectrum of this star shows resonance lines.
- Publication:
-
Istanbul University Faculty Science Review Serie C
- Pub Date:
- 1987
- Bibcode:
- 1987IsRvC..52...45T
- Keywords:
-
- B Stars;
- Shell Stars;
- Stellar Spectra;
- Ultraviolet Spectra;
- Iue;
- Radial Velocity;
- Stellar Atmospheres;
- Stellar Winds;
- Astrophysics;
- Be Stars:Line Identifications;
- Be Stars:UV Spectra;
- Line Identifications:Be Stars;
- UV Spectra:Be Stars