Light Curve Parameters of Cepheid and RR Lyrae Variables at MultipleWavelengths - Models vs. Observations

Singh, H. P. and Das, Susmita and Bhardwaj, A. and Kanbur, S. and Marconi, M. (2019) Light Curve Parameters of Cepheid and RR Lyrae Variables at MultipleWavelengths - Models vs. Observations. BULLETIN DE LA SOCIÉTÉ ROYALE DES SCIENCES DE LIÉGE, 88. pp. 95-102. ISSN 0037-9565

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Abstract

We present results from a comparative study of light curves of Cepheid and RR Lyrae stars in the Galaxy and the Magellanic Clouds with their theoretical models generated from the stellar pulsation codes. Fourier decomposition method is used to analyse the theoretical and the observed light curves at multiple wavelengths. In case of RR Lyrae stars, the amplitude and Fourier parameters from the models are consistent with observations in most period bins except for low metal-abundances (Z < 0:004). In case of Cepheid variables, we observe a greater offset between models and observations for both the amplitude and Fourier parameters. The theoretical amplitude parameters are typically larger than those from observations, except close to the period of 10 days. We find that these discrepancies between models and observations can be reduced if a higher convective efficiency is adopted in the pulsation codes. Our results suggest that a quantitative comparison of light curve structure is very useful to provide constraints for the input physics to the stellar pulsation models.

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