The Ca II infrared triplet as indicator of anomalous Ca isotopic mixture in HgMn stars

Astronomy and Astrophysics – Astrophysics

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Stars: Abundances, Stars: Atmospheres, Stars: Chemically Peculiar, Stars: Atomic Data, Stars

Scientific paper

For the first time we present observational evidence for an anomalous isotopic structure of Ca II in mercury-manganese (HgMn) stars. The centroid wavelengths of Ca II infrared triplet lines in a number of stars have been found redshifted with respect to the centroids of the terrestrial Ca II lines. The record holder is the star HD 175640 for which the measured wavelength is consistent with Ca II being present in the atmosphere entirely in form of the heaviest stable isotope 48Ca. This is a very striking result as 48Ca makes up only 0.187% of the terrestrial Ca mixture.
Based on observations obtained at the European Southern Observator, La Silla and Paranal, Chile (ESO programme Nos. 65.L-0316 and 67.D-0579).

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