Rotational splitting and asteroseismic modelling of the delta Scuti star EE Camelopardalis
arXiv:1702.07428 · doi:10.3847/1538-4357/aa6339
Abstract
According to the rotational splitting law of g modes, the frequency spectra of EE Cam can be disentangled only with oscillation modes of = 0, 1, and 2. Fifteen sets of rotational splits are found, containing five sets of multiplets and ten sets of multiplets. The rotational period of EE Cam is deduced to be = days. When we do model fittings, we use two nonradial oscillation modes ( and ) and the fundamental radial mode . The fitting results show that of the best-fitting model is much smaller than those of other theoretical models. The physical parameters of the best-fitting model are = 2.04 , , = 6433 K, = 1.416, = 4.12 , = 3.518, and = 0.00035. Furthermore, we find and are mixed mode, which mainly characterize the features of the helium core. The fundamental radial mode mainly restrict the features of the stellar envelope. Finally, the acoustic radius and the period separation are determined to be 5.80 hr and 463.7 s respectively, and the size of the helium core of EE Cam is estimated to be = 0.181 and = 0.0796 .
9 pages, 5 figures, 4 tables. accepted for publication in The Astrophysical Journal
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