Long-term Stellar Variations Determined by UV Emission Lines

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Session 46 -- Late Type Stars
Display presentation, Wednesday, 9:20-6:30, Heller Lounge Room

[46.10] Long-term Stellar Variations Determined by UV Emission Lines

J. Mena-Werth, A. Peck, K. Stahl, and R. Price (U. Nebraska at Kearney)

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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