Long-term Stellar Variations Determined by UV Emission Lines

Details Long-term Stellar Variations Determined by UV Emission Lines Long-term Stellar Variations Determined by UV Emission Lines

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aas...182.4610m&link_type=abstract

American Astronomical Society, 182nd AAS Meeting, #46.10; Bulletin of the American Astronomical Society, Vol. 25, p.875

Astronomy and Astrophysics

Astronomy

Scientific paper

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.

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