The Blazhko modulation of TV Boo in 2010
Abstract
We present the analysis of the multicolour CCD observations in the 2010 season of the Blazhko RRc star TV Boo. TV Boo shows a complex Blazhko modulation dominated by two independent modulations with P_{fm1}=9.74 d and P_{fm2}=21.43 d long periods. Both modulation components appear in the frequency spectra as multiplet structures around the harmonics of the pulsation. The positive value of the asymmetry parameter (Q=+0.51) of the primary modulation suggests that it is similar in its character to the Blazhko effect of most of the modulated RRab stars. Interestingly, the secondary, lower-amplitude modulation exhibits a negative asymmetry parameter (Q=-0.22), which is an unusually low value when compared to the Blazhko-modulated RRab stars. Apart from the two modulation frequencies, the spectra also show an additional frequency f' and its linear combinations with the pulsation and the primary modulation f_{1}+f' and f_{1}-f'-f_{m1}. We conclude that the additional frequency most probably belongs to a non-radial mode.
Keywords
Cite
@article{arxiv.1211.3640,
title = {The Blazhko modulation of TV Boo in 2010},
author = {G. Hajdu and J. Jurcsik and Á. Sódor and B. Szeidl and P. Smitola and B. Belucz and K. Posztobányi and K. Vida and E. Kun},
journal= {arXiv preprint arXiv:1211.3640},
year = {2015}
}
Comments
4 pages, 2 figures, accepted for publication in Astronomical Notes, proceedings of "The New Era of Helio- and Asteroseismology", 2012. 05. 20-25. Obergurgl (A)