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S. R. Cortes, J. R. King (Clemson University)
A photometric investigation of three blue stars of low iron abundance was conducted during the summer of 2003; the goal was to determine if a periodic variation in brightness exists. The observations were taken with the SARA 0.9m telescope during three nights at the end of June for the stars CS22890-069 and CS22872-062, and data taken during one night in the beginning of July for the star CS22884-065. This project was made possible by the National Science Foundation with grant AST0097616, the Curry Foundation, and the Shodor Foundation.
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Bulletin of the American Astronomical Society, 35#5
© 2003. The American Astronomical Soceity.