Volume 380, Number 1, December II 2001
|Page(s)||286 - 291|
|Section||Stellar structure and evolution|
|Published online||15 December 2001|
HD 174005: Another binary classified as λ Bootis*
Dipartimento di Astronomia, Università degli Studi di Trieste, Via G. B. Tiepolo 11, 34131 Trieste, Italy e-mail: email@example.com
2 Institut d'Astrophysique, 98bis Bld. Arago 75014 Paris, France e-mail: firstname.lastname@example.org
3 Université de Paris Sud XI, France
4 Istituto Nazionale per l'Astrofisica - Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34131 Trieste, Italy e-mail: email@example.com
Corresponding author: R. Faraggiana, firstname.lastname@example.org
Accepted: 10 October 2001
We demonstrate that HD 174005, a star recently classified as belonging to the λ 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.
Key words: stars: atmospheres / stars: chemically peculiar / stars: binaries: spectroscopic
© ESO, 2001
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