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摘要:
We present the dependence of electron temperature fluctuations of O++ and H+ by the chemical abundances of oxygen and nitrogen. Models assume that hydrogen density is uniform in one case and non uniform in the second case, which vary with the distance from the central star. The abundances of oxygen and nitrogen change by scale factor 5 and 1/5. Our analysis suggests that temperature fluctuations are consistent with photoionization. Using the cloudy photoionization code, we found a reasonable close agreement of the computed value with the one that was done before this work. Our simulation also shows that how change of abundances affects temperature fluctuations and its value is less than 0.01.
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篇名 Temperature Fluctuations in Photoionized Nebulae in Case of Oxygen and Nitrogen Abundances
来源期刊 应用数学(英文) 学科 数学
关键词 H II REGION PLANETARY NEBULAE ABUNDANCES
年,卷(期) 2015,(2) 所属期刊栏目
研究方向 页码范围 440-446
页数 7页 分类号 O1
字数 语种
DOI
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H
II
REGION
PLANETARY
NEBULAE
ABUNDANCES
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研究分支
研究去脉
引文网络交叉学科
相关学者/机构
期刊影响力
应用数学(英文)
月刊
2152-7385
武汉市江夏区汤逊湖北路38号光谷总部空间
出版文献量(篇)
1878
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0
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