Fig. 1
Spectra of CD-41°15048 (top) and HD 214362 (bottom). Absorption lines due to the transitions of Ca i 6122.23, Fe i 6137.70, and Ba ii 6141.73 are also shown. Dashed lines represent their rest wavelengths. The spectral lines are shifted towards the red by about 4.6 Å for CD-41°15048 due to a RV of 228.9 ± 0.6 km s-1. For HD 214362, the absorption lines are shifted towards the blue by about 2.0 Å due to a RV of −92.4 ± 0.7 km s-1.
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