The 65.767-day brightness cycle of the Herbig AeBe star R CrA is best explained by a close binary (about 3.0 and 2.3 solar masses) partially hidden by a circumbinary disk, with secular dimming from disk precession.
A., Herbst , W., Hughes , A
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The origin of R CrA variability: A complex triple system hosting a disk
The 65.767-day brightness cycle of the Herbig AeBe star R CrA is best explained by a close binary (about 3.0 and 2.3 solar masses) partially hidden by a circumbinary disk, with secular dimming from disk precession.