Abstract
ABSTRACTGSC 2985‐01044 is a δ Scuti star with a period of 0.0933584 days and a V‐magnitude range of 11.85–12.05; its light curve is slightly variable. The location, space motion, and other properties of this star indicate that it is a higher amplitude δ Scuti star (or “dwarf Cepheid”) that is a member of the old disk population. The problem of determining the local space densities of the various populations of the higher amplitude δ Scuti stars is discussed.
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