EE PEGASI REVISITED: A SPECTRUM SYNTHESIS AND NEW LIGHT SYNTHESIS STUDY

A. P. LINNELL; I. HUBENY; C. H. S. LACY

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EE PEGASI REVISITED: A SPECTRUM SYNTHESIS AND NEW LIGHT SYNTHESIS STUDY

机译：EE PEGASI修订：光谱合成和新光合成研究

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A self-consistent physical model, described in an earlier paper by Linnell & Hubeny, has permitted fits of synthetic spectra to observed spectra of EE Pegasi. The synthetic spectra determine abundances for iron, calcium, and silicon. The same model has been the basis of an optimized light synthesis solution of an accurate light curve by Ebbighausen. The solution, requiring use of a model atmospheres option to represent the component star radiative properties, agrees with the standard solution by Lacy & Popper. The derived component parameters place them on an isochrone, determine a compositional Z, and are in accordance with evolution tracks by Schaller et al. The model is not restricted to systems with small distortion.

机译：Linnell＆Hubeny在较早的论文中描述了一个自洽的物理模型，该模型允许合成光谱与EE Pegasi的观测光谱拟合。合成光谱确定铁，钙和硅的丰度。相同的模型是Ebbighausen优化的精确光曲线的光合成解决方案的基础。该解决方案需要使用模型大气选项来表示组件星的辐射特性，因此与Lacy＆Popper的标准解决方案一致。导出的成分参数将它们放置在等时轴上，确定组成Z，并与Schaller等人的演化轨迹一致。该模型不限于失真小的系统。

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《The Astrophysical journal》 |1996年第2pt1期|p.721-728|共8页
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A. P. LINNELL; I. HUBENY; C. H. S. LACY;
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EE PEGASI REVISITED: A SPECTRUM SYNTHESIS AND NEW LIGHT SYNTHESIS STUDY

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