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A&A 367, 831-839 (2001)
DOI: 10.1051/0004-6361:20000531
Spectroscopic investigations of classical Cepheids and main-sequence stars in galactic open clusters and associations
I. Association Cas OB2 and the small-amplitude Cepheid SU Cassiopeae
I. A. Usenko1, 2, V. V. Kovtyukh1, 2, V. G. Klochkova3, 4, V. E. Panchuk3, 4 and S. V. Yermakov31 Astronomical Observatory of Odessa State University, Odessa 65014, Ukraine
e-mail: val@deneb.odessa.ua
2 Isaac Newton Institute of Chile, Odessa Branch
3 Special Astrophysical Observatory, Russian Academy of Sciences, Nizhny Arkhyz, Stavropol Territory, 369167, Russia
e-mail: valenta@sao.ru; panchuk@sao.ru; ermak@sao.ru
4 Isaac Newton Institute of Chile, SAO RAS Branch
(Received 13 July 2000 / Accepted 17 November 2000)
Abstract
The small-amplitude Cepheid SU Cas and four members of
the association Cas OB2 (HD 16893, HD 17327a and
b
, HD 17443) were investigated, using high-resolution
CCD spectra. The following results were obtained: 1) All
these objects have the same metallicity values, close to that of the
Sun; 2) Elemental abundance indicates that SU Cas is a
post first dredge-up star with an age from 1 108 to
1.45 108 yr, and it is not crossing the Cepheid
instability strip for the first time. The mean value of
=
2.35 corresponds to pulsations in the fundamental tone, although errors
in gravity estimations provide overtone pulsations. The questions
about its pulsational mode and membership in Cas OB2
remained open; 3) HD 17327a is a slowly rotating
HgMn-star with the highest helium content among such
objects, while HD 16893 also has a manganese overabundance
and might be classified as an Am-star; 4) HD 17327b
and HD 17443 are rapidly rotating main-sequence stars,
while HD 17443 has a helium content comparable with that of the Sun.
Key words: associations -- stars: abundances -- stars: Cepheids -- stars: main-sequence
Offprint request: I. A. Usenko, igus@deneb.odessa.ua
SIMBAD Objects in preparation
© ESO 2001
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