We present an analysis of nine bright spectroscopic binaries (HD 1585, HD 6613, HD 12390, HD 39923, HD 55201, HD 147430, HD 195543, HD 202699, HD 221643), which have orbital periods of
days. These well‐separated binaries are the last stars of our sample that we observed with the TIGRE telescope obtaining intermediate‐resolution spectra of
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