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A&A 412, 447-464 (2003)
DOI: 10.1051/0004-6361:20031472
The heterogeneous class of
Bootis stars
M. Gerbaldi1, 2, R. Faraggiana3 and O. Lai4
1 Institut d'Astrophysique, 98bis Bd. Arago, 75014 Paris, France
2 Lab. Astronomie, Bât. 470, Université de Paris Sud XI, 91405 Orsay Cedex, France
3 Dipartimento di Astronomia, Università degli Studi di Trieste, via G.B. Tiepolo 11, 34131 Trieste, Italy
e-mail: faraggiana@ts.astro.it
4 Canada-France-Hawaii Telescope (CFHT) Corporation, Kamuela, HI 96743, USA
e-mail: lai@cfht.hawaii.edu
(Received 10 June 2003 / Accepted 12 September 2003 )
Abstract
We demonstrate that it is arduous to define the
Boo stars
as a class of objects exhibiting uniform abundance peculiarities which
would be generated by a mechanism altering the structure of their
atmospheric layers.
We collected the stars classified as
Boo up to now and discuss their
properties, in particular the important percentage of confirmed binaries
producing composite spectra (including our adaptive optics observations)
and of misclassified objects.
The unexplained
RV variables (and thus suspected binaries), the known SB for
which we lack information on the companion,
the stars with an UV flux
inconsistent with their classification, and the
fast rotating stars for which
no accurate abundance analysis can be performed, are also reviewed.
Key words: stars: atmospheres -- stars: chemically peculiar -- stars: binaries: spectroscopic
Offprint request: M. Gerbaldi, gerbaldi@iap.fr
SIMBAD Objects
© ESO 2003
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