Low-resolution spectral classification of very faint emission-line galaxies

被引：3
作者：
Murayama, T [1 ]
Taniguchi, Y [1 ]
机构：
[1] Tohoku Univ, Inst Astron, Aoba Ku, Sendai, Miyagi 9808578, Japan
来源：
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN | 1998年 / 50卷 / 02期
关键词：
galaxies; active; Seyfert; interstellar; H II regions;
D O I：
10.1093/pasj/50.2.241
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
In order to classify the emission-line activity of very faint galaxies, we present a new classification method based on low spectral-resolution (lambda/Delta lambda similar to 50) spectroscopic data. Our new method enables us to classify faint emission-line objects with B < 26, which will be obtained by using deep optical and near-infrared spectroscopy with an 8-m class of telescope facilities.
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页码：241 / 248
页数：8
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