The Fe II 6149 A line in the HgMn star MU Leporis - Can the star's magnetic field be detected?

Statistics – Computation

Scientific paper

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Iron, Line Spectra, Metallic Stars, Peculiar Stars, Stellar Magnetic Fields, Abundance, Computational Astrophysics, Data Reduction, Spectral Line Width, Spectral Resolution

Scientific paper

The anomalous strength of the Fe II 6149 A line relative to the Fe II 6147 A line is confirmed in the spectrum of Mu Leporis and turns out to be caused by a blending with the Hg II 6149.5 A line. This fact reveals that a magnetic field in Mu Lep cannot be reliably detected using the empirical relation for the correlation of magnetic-field strength with the difference between the equivalent widths of the two Fe II lines.

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