CAOSP abstracts, Volume: 38, No.: 2, year: 2008

Abstract: We present the preliminary results of a spectral analysis of the HgMn star HR 4817. The abundance calculation is obtained by comparing observed with synthetic spectra. We compare the results with our previous analyses of the same star. The abundances are more accurate and we found elements we didn't find in our previous analyses.

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Last update: April 17, 2008