@misc{10481/89083,
year = {2009},
url = {https://hdl.handle.net/10481/89083},
abstract = {We present an analysis of the δ-Scuti star HD 174936 (ID 7613) 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 μHz. 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.},
publisher = {EDP Sciences},
title = {Asteroseismic analysis of the CoRoT δ Scuti star HD 174936},
doi = {10.1051/0004-6361/200911932},
author = {García Hernández, Antonio and Moya, Andrés and Garrido, R. and Suárez Yanes, Juan Carlos and Rodríguez, E. and Amado, P. J. and Martín Ruiz, Sergio and Rolland Quintanilla, Ángel},
}