Statistics – Computation
Scientific paper
Feb 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992pasp..104..106t&link_type=abstract
Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 104, Feb. 1992, p. 106-110.
Statistics
Computation
10
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.
Jugaku Jun
Takada-Hidai Masahide
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