Long-term Stellar Variations Determined by UV Emission Lines
Abstract
Using the IUE archive, main sequence stars are selected which have spectral observations throughout the sixteen year history of the satellite. Emission line fluxes are measured to determine if long-term stellar variation is evident. Our results are then compared to those derived by O. Wilson and A. Vaughan.
- Publication:
-
American Astronomical Society Meeting Abstracts #182
- Pub Date:
- May 1993
- Bibcode:
- 1993AAS...182.4610M