作者: G. Tagliaferri , L. Pastori , G. Cutispoto , R. Pallavicini
DOI: 10.1017/S0074180900166884
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摘要: We selected a sample of active cool stars detected in the EUV band by ROSAT WFC and performed spectroscopic photometric observations. inferred spectral type, luminosity class, distance, binary status, rotational velocity. Here we show results Li abundances determination from I 6707.8 A line.