Stellar Variability in the Lower Part of the Instability Strip

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The photometric properties of the variable stars located in the lower part of the classical instability strip are discussed. The importance of the determination of some light curve parameters and their connection with the stellar models are stressed, with a particular emphasis on large amplitude Delta Sct (DSCT) stars.
4 pages, 1 figure. LaTeX (paspconf.sty). To be published in the proceedings of the 86th AAVSO Spring Meeting `Variable Stars: New Frontiers', Astronomical Society Pacific Conference Series

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