Volume 425, Number 2, October II 2004
|Page(s)||615 - 626|
|Section||Stellar structure and evolution|
|Published online||21 September 2004|
Bootis stars with composite spectra*
Dipartimento di Astronomia, Università degli Studi di Trieste, via G.B. Tiepolo 11, 34131 Trieste, Italy e-mail: firstname.lastname@example.org
2 Istituto Nazionale per l'Astrofisica – Osservatorio Astronomico di Trieste, via G.B. Tiepolo 11, 34131 Trieste, Italy
3 Institut d'Astrophysique, 98 bis Bd. Arago, 75014 Paris, France
4 Université de Paris Sud XI, France
Accepted: 3 June 2004
We examine the large sample of λ Boo candidates collected in Table 1 of Gerbaldi et al. ([CITE]) to see how many of them show composite spectra. Of the 132 λ Boo candidates we identify 22 which definitely show composite spectra and 15 more for which there are good reasons to suspect a composite spectrum. The percentage of λ Boo candidates with composite spectra is therefore >17% and possibly considerably higher. For such stars the λ Boo classification should be reconsidered taking into account the fact that their spectra are composite. We argue that some of the underabundances reported in the literature may simply be the result of the failure to consider the composite nature of the spectra. This leads to the legitimate suspicion that some, if not all, the λ Boo candidates are not chemically peculiar at all. A thorough analysis of even a single one of the λ Boo candidates with composite spectra, in which the composite nature of the spectrum is duly considered, which would demonstrate that the chemical peculiarities persist, would clear the doubt we presently have that the stars with composite spectra may not be λ Boo stars at all.
Key words: stars: atmospheres / stars: chemically peculiar / stars: binaries: spectroscopic / stars: fundamental parameters / binaries: visual / stars: abundances
© ESO, 2004
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