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Post-Asymptotic Giant Branch Evolution of Low- and Intermediate-Mass Stars. Preliminary Results

机译:低渐近巨型巨型分支演化,低级群众旗帜。初步结果

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Preliminary results from an ongoing project to compute a grid of post-AGB models is presented. Our preliminary results show that stellar evolution computations that include an updated treatment of the microphysics predict post-AGB timescales that are several times shorter that predicted by older models. Also the mass-luminosity relation of post-AGB models deviates from that of older grids. In addition, our results suggest only a slight metallicity dependence of the post-AGB timescales. We expect these results to have significant consequences for models of the formation of planetary nebulae and their luminosity function.
机译:提出了持续项目来计算AGB模型网格网格的初步结果。我们的初步结果表明,恒星演化计算包括更新的微妙物理治疗预测较旧模型预测的较短的AGB时间尺寸。此外,AGB模型的质量亮度关系偏离旧网格的关系。此外,我们的结果表明,AGB时间尺寸的略微金属性依赖性。我们预计这些结果对于形成行星星云的模型及其亮度函数具有重大影响。

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