Emission from an inhomogeneous plasma: Line intensities and determination of elemental abundances in gaseous nebulae with fluctuations of Te and ne

被引：2

作者：

Kholtygin A.F. ^{[1
]}

机构：

[1] Astronomical Institute, St. Petersburg State University

来源：

Astrophysics | 2000年 / 43卷 / 4期

关键词：

Distribution Function; Chemical Element; Mass Density; Line Intensity; Actual Distribution;

D O I：

10.1023/A:1010975110093

中图分类号：

学科分类号：

摘要：

A method is proposed for determining the abundances of chemical elements in planetary nebulae based on allowance for the actual distribution functions of errors in measuring line intensities. Fluctuations both in temperature and in mass density of a nebula are taken into account in the proposed method. The results of a determination of C and O abundances and of the amplitudes of temperature and density fluctuations are given. ©2000 Kluwer Academic/Plenum Publishers.

引用

页码：463 / 473

页数：10

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