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EW and chemical abundances in 211 stars with HARPS

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B2FIND2026-03-19 收录
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https://b2find.eudat.eu/dataset/9c301b30-02d3-5a15-b065-e7865d28a500
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Magnetic fields and stellar spots can alter the equivalent widths of absorption lines in stellar spectra, varying during the activity cycle. This also influences the information...
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