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The chemical composition of galactic planetary nebulae with regard to inhomogeneity in the gas density in their envelopes

机译:银河系行星状星云的化学成分,关于其包壳中气体密度的不均匀性

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The results of a study of the chemical compositions of Galactic planetary nebulae taking into account two types of inhomogeneity in the nebular gas density in their envelopes are reported. New analytical expressions for the ionization correction factors have been derived and are used to determine the chemical compositions of the nebular gas in Galactic planetary nebulae. The abundances of He, N, O, Ne, S, and Ar have been found for 193 objects. The Y-Z diagrams for various He abundances are analyzed for type II planetary nebulae separately and jointly with HII regions. The primordial helium abundance Y-p and enrichment ratio dY/dZ are determined, and the resulting values are compared with the data of other authors. Radial abundance gradients in the Galactic disk are studied using type II planetary nebulae. (C) 2005 Pleiades Publishing, Inc.
机译:报告了银河系行星状星云化学成分研究的结果,其中考虑到了它们包膜中的两种星状气体密度的不均匀性。已经推导了电离校正因子的新分析表达式,并用于确定银河系行星状星云中星云气体的化学成分。已发现193个对象的He,N,O,Ne,S和Ar的丰度。分别分析II型行星状星云以及与HII区域一起分析的各种He丰度的Y-Z图。确定了原始氦的丰度Y-p和富集比d​​Y / dZ,并将所得值与其他作者的数据进行了比较。使用II型行星状星云研究了银河系盘中的径向丰度梯度。 (C)2005年Pleiades Publishing,Inc.

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