Journal
ASTRONOMY & ASTROPHYSICS
Volume 506, Issue 1, Pages 79-83Publisher
EDP SCIENCES S A
DOI: 10.1051/0004-6361/200911932
Keywords
delta Sct; stars: rotation; stars: oscillations; stars: fundamental parameters; stars: interiors
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Funding
- Spanish Plan Nacional del Espacio [ESP2007-65480-C02-01]
- Spanish Ministry of Science and Innovation
- Consejo Superior de Investigaciones Cient ficas
- European Social Fund
- Italian ESS [ASI/INAFI/015/07/0, WP 03170]
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We present an analysis of the delta-Scuti star HD 174936 (ID7613) observed by CoRoT during the first short run SRc01 ( 27 days). A total number of 422 frequencies were extracted from the light curve using standard prewhitening techniques. This number of frequencies was obtained by considering a spectral significance limit of sig = 10 using the software package SigSpec. Our analysis of the oscillation frequency spectrum reveals a spacing periodicity around 52 mu Hz. Although modes considered here are not in the asymptotic regime, a comparison with stellar models confirms that this signature may stem from a quasi-periodic pattern similar to the so-called large separation in solar-like stars.
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