Further investigations of R Aquilae

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Scientific paper

R Aquilae is well known as a Mira variable of ever decreasing period. Statistical tests upon, and descriptive analyses of, this star are conducted. Conclusions are drawn regarding the significance of R Aquilae's variation in period. Since this star's change in period is so conspicuous, it serves as a baseline against which the results for other Miras can be compared.

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