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<p>the period of <a href="page.php?w=rotation">rotation</a> of the star. It is thought that they are caused by an inhomogeneous distribution of chemical elements in the <a href="page.php?w=stellar_atmosphere">atmosphere</a>s of these stars. These result in spots and enhanced element abundances, which produce localized variations in surface flux. The <a href="page.php?w=oblique_rotator_model">oblique rotator model</a> explains how these variations are carried across the field of view, resulting in the stellar variability. Several factors are thought</p><p>
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