The triple-mode pulsating variable V823 Cas
Abstract
Based on extended multicolour CCD photometry of the triple-mode radial pulsator V823 Cas we studied the properties of the coupling frequencies invoked by nonlinear processes. Our results support that a resonance connection as suggested by Antonello & Aikawa (1998) affects the mode coupling behaviour. The P1/P0 period ratio of V823 Cas has an "out of range" value if compared with the period ratios of the known double mode pulsators, while the P2/P1 period ratio is normal. The periods and period ratios cannot be consistently interpret without conflict with pulsation and/or evolution models. We attempt to interpret this failure by the suggestion that at present, the periods of V823 Cas are in a transient, resonance affected state, thus do not reflect the true parameters of the object. The anomalous period change behaviour of the fundamental and second overtone modes supports this idea. We have also raised the possibility that a f0 + f2 = 2f1 resonance may act in triple mode pulsators.
Cite
@article{arxiv.astro-ph/0508646,
title = {The triple-mode pulsating variable V823 Cas},
author = {J. Jurcsik and B. Szeidl and M. Váradi and A. Henden and Zs. Hurta and B. Lakatos and K. Posztobányi and P. Klagyivik and Á. Sódor},
journal= {arXiv preprint arXiv:astro-ph/0508646},
year = {2009}
}
Comments
10 pages, 7 figures, 5 tables. Accepted for publication in Astronomy and Astrophysics