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• W3100263819 endingPage "863" @default.
• W3100263819 startingPage "851" @default.
• W3100263819 abstract "Chemically peculiar (CP) stars are unique natural laboratories for investigation of the microscopic diffusion processes of chemical elements. The element segregation under the influence of gravity and radiation pressure leads to the appearance of strong abundance gradients in the atmospheres of CP stars. Consequently, the atmospheric temperature-pressure structure of these objects could deviate significantly from the atmospheres of normal stars with homogeneous abundances. In this study we performed a self-consistent, empirical model atmosphere study of the brightest rapidly oscillating Ap star alpha Cir. We account for chemical stratification in the model atmosphere calculations and assess the importance of non-uniformed vertical element distribution on the model structure, energy distribution and hydrogen line profiles. Based on an iterative procedure of the chemical abundance analysis of 52 ions of 35 elements, stratification modeling of 4 elements (Si, Ca, Cr and Fe) and subsequent re-calculations of the atmospheric structure, we derived a new model atmosphere of alpha Cir, which is consistent with the inferred atmospheric chemistry of the star. We find Teff=7500 K, logg=4.1, and demonstrate that chemical stratification has a noticeable impact on the model structure and modifies the formation of the hydrogen Balmer lines. Our spectroscopically determined Teff of alpha Cir agrees with the fundamental effective temperature of this star. This shows that temperatures inferred in detailed spectroscopic analyses of cool magnetic CP stars are not affected by a large systematic bias." @default.
• W3100263819 created "2020-11-23" @default.
• W3100263819 creator A5037297844 @default.
• W3100263819 creator A5042408274 @default.
• W3100263819 creator A5056341479 @default.
• W3100263819 date "2009-04-08" @default.
• W3100263819 modified "2023-09-23" @default.
• W3100263819 title "A self-consistent empirical model atmosphere, abundance and stratification analysis of the benchmark roAp star<i>α</i> Circini" @default.
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• W3100263819 doi "https://doi.org/10.1051/0004-6361/200911653" @default.
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