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Isotopic composition of Hg and Pt in slowly rotating HgMn stars

S. Hubrig, F. Castelli, G. Mathys

astro-pharXiv:astro-ph/9805189

Abstract

Preliminary results from a study of the isotopic compositions of the elements Hg and Pt in a number of HgMn stars are presented. This work represents an improvement over previous studies thanks to the very high spectral resolution available (R = 118 000) and to the new information on wavelengths and atomic structure of Hg II and Pt II.

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