Delta Scuti stars are a type of pulsating variable star that exhibit small amplitude brightness variations due to non-radial pulsations. These stars are typically located on the instability strip of the Hertzsprung-Russell diagram and are primarily young, hot, and often found in the spectral types A and F. Their variability is linked to their internal structure and stellar evolution, making them an important subject of study in understanding stellar pulsations and the physical processes within stars.
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