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On the new late B- and early A-type periodic variable stars

By Nami Mowlavi and others
We summarize the properties of the new periodic, small amplitude, variable stars recently discovered in the open cluster NGC 3766. They are located in the region of the Hertzsprung-Russell diagram between \delta\ Sct and slowly pulsating B stars, a region where no sustained pulsation is predicted by standard models. The... Show more
January 8, 2014
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On the new late B- and early A-type periodic variable stars
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