The third spectrum of Erbium in HR 465

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Abundance, Erbium, Peculiar Stars, Stellar Composition, Stellar Spectra, Dysprosium, Iue, Line Spectra, Ultraviolet Spectra

Scientific paper

The strong presence of Er III in coude spectra of the chemically peculiar (CP) A star HR 465 at the time of rare-earth maximum is discussed. Er III is surely present in other CP stars; earlier studies are confirmed. Er III is only a marginal detection on IUE images of HR 465. A very crude abundance calculation, using an assumed oscillator strength for a 'typical' line gives a value for erbium some two orders of magnitude below earlier results based on Er II. An incidental identification, Dy III in gamma Equ, is briefly discussed.

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