HD 174005: another binary classified as lambda Boo
Astrophysics
2009-11-07 v1
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.
Cite
@article{arxiv.astro-ph/0110574,
title = {HD 174005: another binary classified as lambda Boo},
author = {R. Faraggiana and M. Gerbaldi and P. Bonifacio},
journal= {arXiv preprint arXiv:astro-ph/0110574},
year = {2009}
}
Comments
Accepted by A&A