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

For the first time we present observational evidence for an anomalous isotopic structure of Ca  in mercury-manganese (HgMn) stars. The centroid wavelengths of Ca  infrared triplet lines in a number of stars have been found redshifted with respect to the centroids of the terrestrial Ca  lines. The record holder is the star HD 175640 for which the measured wavelength is consistent with Ca  being present in the atmosphere entirely in form of the heaviest stable iso- tope 48 Ca. This is a very striking result as 48 Ca makes up only 0.187% of the terrestrial Ca mixture.