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Rotating ellipsoidal variables are a class of close binary variable star systems whose components are ellipsoidal. They are not eclipsing, but fluctuations in apparent magnitude occur due to changes in the amount of light emitting area visible to the observer. Typical brightness fluctuations do not exceed 0.1 magnitudes.
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ellipsoidal variable variables rotating fluctuations star light binary spica class close systems whose components eclipsing apparent magnitude occur due changes
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