Issue |
A&A
Volume 450, Number 2, May I 2006
|
|
---|---|---|
Page(s) | 715 - 723 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361:20053942 | |
Published online | 10 April 2006 |
The frequency ratio method and the new multiperiodic γ Doradus star HD 218427
1
Instituto de Astrofísica de Andalucía, CSIC, PO Box 3004, 18080 Granada, Spain e-mail: eloy@iaa.es
2
European Southern Observatory, Alonso de Cordova 3107, Santiago 19, Chile
3
LESIA, Observatoire de Paris-Meudon, UMR 8109, 92190 Meudon, France
4
INAF-Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807 Merate, Italy
5
CRAAG, Algiers Observatory, BP 63 Bouzareah, 16340 Algiers, Algeria
Received:
29
July
2005
Accepted:
1
January
2006
Oscillations of γ Dor-type were discovered in the star HD 218427
through simultaneous uvby photometric observations carried out in the
year 2003. A few
H-Crawford measurements were also collected for calibration
purposes and they locate this star well
inside the γ Dor instability region. We find HD 218427 to be deficient
in metals, similar to other well-defined γ Dor stars, and discuss the
possibility that it has a λ Boo nature. We carried out frequency
analysis for different filters, including the combined “vby” filter, and
five frequencies were found as significant with periods ranging between 0.3
and 0.8 days. The recently-developed frequency ratio method is used in order
to identify the excited modes. The results are consistent
with an
identification for all the modes and with high radial
quantum numbers (
) for the three main observed periodicities.
The
possibility of multiplet structures is also discussed.
However, no consistency is found when using the time-dependent convection
treatment to discriminate modes.
This disagreement can be due to the large rotation velocity taking place in
HD 218427 and, consequently, the significant coupling between the modes.
Key words: stars: variables: general / stars: individual: HD 218427 / stars: oscillations / techniques: photometric
© ESO, 2006
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.