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- W2158741344 abstract "The anomalous strength of the Fe II 6147:7 line relative to Fe II 6149:2 in the stars with magnetic fields is used for detecting magnetic fields in very slowly rotating HgMn stars. The diagnosis based on this pair of magnetically sensi- tive Fe lines is a simple and fast tool, but its application to more rapidly rotating HgMn stars is hampered by blending with Hg II 6149:5. For spectra of sharp-lined HgMn stars (with v sin i< 4 km s 1 ) taken at high resolving power (R100000) both lines, Fe II 6149:25 and Hg II 6149:48, become fully unblended. The observed relative differences between the equiv- alent widths of the two Fe II lines are compared with those de- rived from synthetic spectra computed by neglecting magnetic field effects. This comparison has shown that three HgMn stars, HD 175640, HD 178065 and HD 186122 are very likely to pos- sess a magnetic field that could be larger than 2 kG." @default.
- W2158741344 created "2016-06-24" @default.
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- W2158741344 date "1999-06-01" @default.
- W2158741344 modified "2023-09-27" @default.
- W2158741344 title "Search for magnetic fields in HgMn stars by using relative strengths of multiplet 74 Fe II lines" @default.
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- W2158741344 hasPublicationYear "1999" @default.
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