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Because they are close to the ecliptic, these stars can be occulted by the Moon and, very rarely, by planets.
References
Trunkovskij, E. M. (October 1987), "Stellar angular dimensions obtained by the lunar occultation technique", Pis'ma Astron. Zu., 13: 900–906, Bibcode:1987PAZh...13..900T.
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