The Abundance Ratio C/O in the Atmospheres of 89 Carbon Stars

被引：0

作者：

I. Eglitis

M. Eglite

机构：

[1] Latvian Academy of Sciences,Radioastrophysical Observatory

来源：

Astrophysics and Space Science | 1997年 / 249卷

关键词：

Abundance Ratio; Carbon Star; Visual Magnitude; Byurakan Astrophysic Observatory; Heavy Element Abundance;

D O I：

暂无

中图分类号：

学科分类号：

摘要：

The abundance ratio C/O in the atmospheres of 89 faint carbon stars are detected on the basis of spectra obtained on 2.6 m telescope of Byurakan AO. The frequency distribution of C/O in the Perseus galactic arm differs from that in the Orion arm. The conclusion is made that the reason of the difference may be the heavy element abundance differences in these galactic arms.

引用

页码：235 / 256

页数：21

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