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International Ultraviolet Explorer satellite observations of seven high-excitation planetary nebulae

机译:国际紫外线探测卫星对七个高激发行星状星云的观测

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摘要

Observations of seven high-excitation planetary nebulae secured with the International Ultraviolet Explorer (IUE) satellite were combined with extensive ground-based data to obtain electron densities, gas kinetic temperatures, and ionic concentrations. We then employed a network of theoretical model nebulae to estimate the factors by which observed ionic concentrations must be multiplied to obtain elemental abundances. Comparison with a large sample of nebulae for which extensive ground-based observations have been obtained shows nitrogen to be markedly enhanced in some of these objects. Possibly most, if not all, high-excitation nebulae evolve from stars that have higher masses than progenitors of nebulae of low-to-moderate excitation.
机译:使用国际紫外线探测器(IUE)卫星获得的七个高激发行星状星云的观测结果与广泛的地面数据相结合,以获得电子密度,气体动力学温度和离子浓度。然后,我们使用理论模型星云的网络来估计必须乘以所观察到的离子浓度以获得元素丰度的因素。与已经获得广泛地面观测的大量星云样本进行比较后,发现其中一些物体中的氮显着增强。可能是,即使不是全部,大多数高激发星云都是从质量比低激发到中激发星云的祖先更高的恒星演化而来。

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