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A Determination of the Elements of V493 Aquilae

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Bradley Meyer

Marie Mitchell Observatory, Nantucket, MA 02554

Abstract

The elements of the variable star V943 Aquilae are determined from comparisons with a new set of sequence stars. The period of the star is found to have been constant over the range of years from 1935 to 1975, but to have varied in a slower but undetermined fashion outside this range.