Abstract
Although, in a historical view (see Section 1.1), R Coronae Borealis stars – usually addressed as R CrB stars – were the first kind of objects observed exhibiting pronounced occultations that seemed to appear episodically in their light curves (Figure 18.1). Despite the considerable endeavor in particular in the last century to physically and chemically reveal this conspicuous stellar behavior, there is still no final explanation of these spectacular occultations based on a consistent modeling satisfying all observational and theoretical aspects.
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