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A High‐Resolution Spectrum of the R Coronae Borealis Star V2552 Ophiuchi

Photometry and low‐resolution spectroscopy have added V2552 Oph to the rare class of R Coronae Borealis variables. We confirm this classification of V2552 Oph through a comparison of our high‐resolution optical spectrum of this star and that of R CrB and other F‐type members of the class. We show that V2552 Oph most closely resembles Y Mus and FH Sct, stars in which Sr, Y, and Zr are enhanced.