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arXiv · 1212.0897

V1820 Orionis : an RR Lyrae star with strong and irregular Blazhko effect

Pierre de Ponthiere·Franz-Josef Hambsch·Tom Krajci·Kenneth Menzies·Patrick Wils
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Abstract

The Blazhko effect in V1820 Orionis and its period were reported for the first time by Wils et al. (2006) from a data analysis of the Northern Sky Variability Survey. The results of additional V1820 Orionis observations over a time span of 4 years are presented herein. From the observed light curves, 73 pulsation maxima have been measured. The times of light maxima have been compared to ephemerides to obtain the (O-C) values. The Blazhko period (27.917 +/- 0.002 d) has been derived from light curve Fourier analysis and from ANOVA analyses of the (O-C) values and of magnitudes at maximum light (Mmax). During one Blazhko cycle, a hump in the ascending branch of the light curve was clearly identified and has also created a double maximum in the light curve. The frequency spectrum of the light curve, from a Fourier analysis with Period04, has revealed triplet, quintuplet structures, and a second Blazhko weak modulation (period = 34.72 +/-0.01 d). V1820 Orionis can be ranked as a strongly modulated star based on its observed amplitude and phase variations. The amplitude ratio of the largest triplet component to main pulsation component is quite large: 0.34.

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Pierre de Ponthiere, Franz-Josef Hambsch, Tom Krajci, Kenneth Menzies, Patrick Wils. 2012-12-04. V1820 Orionis : an RR Lyrae star with strong and irregular Blazhko effect. https://arxiv.org/abs/1212.0897

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