HD 174005: another binary classified as lambda Boo
arXiv:astro-ph/0110574 · doi:10.1051/0004-6361:20011440
Abstract
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.
Accepted by A&A