Precision wavelengths for expected emission lines in high-redshift galaxies and quasars

被引：0
|
作者：
Osterbrock, DE [1 ]
机构：
[1] Univ Calif Santa Cruz, Univ Calif Observ, Lick Observ, Santa Cruz, CA 95064 USA
来源：
SIXTH TEXAS-MEXICO CONFERENCE ON ASTROPHYSICS: ASTROPHYSICAL PLASMAS NEAR AND FAR | 1997年 / 7卷
关键词：
galaxies; quasars; emission lines; line; identification; ultraviolet; general;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Precision wavelengths, accurate to 0.01 Angstrom, are listed for the strongest expected ultraviolet emission lines in galaxies (including star-formation regions, Seyfert galaxies and radio galaxies) and quasars, for use in spectra observed either in the UV or optical spectral regions.
引用
收藏
页码：180 / 185
页数：6
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