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2001-10-26
HD 174005: another binary classified as lambda Boo
R. FaraggianaM. GerbaldiP. Bonifacio
文献摘要
We demonstrate that HD 174005, a star recently classified as belonging to the lambda Boo group, is in reality a double lined spectroscopic binary; at some phases, the observed composite spectrum may be similar to that of a single star with weak metal lines.
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