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23 April 2024
 
  » arxiv » astro-ph/9805189

 Article overview


Isotopic composition of Hg and Pt in slowly rotating HgMn stars
S. Hubrig ; F. Castelli ; G. Mathys ;
Date 14 May 1998
Subject astro-ph
Affiliation University of Potsdam, Germany, CNR, Trieste, Italy, ESO, Chile
AbstractPreliminary 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.
Source arXiv, astro-ph/9805189
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