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

页码：180 / 185

页数：6