ISO spectroscopy of galaxies

被引：1
|
作者：
Lutz, D [1 ]
机构：
[1] Max Planck Inst Extraterr Phys, D-85741 Garching, Germany
来源：
NEW RESULTS IN FAR IR AND SUB-MM ASTRONOMY | 2002年 / 30卷 / 09期
关键词：
D O I：
10.1016/S0273-1177(02)00579-3
中图分类号：
V [航空、航天];
学科分类号：
08 ; 0825 ;
摘要：
Mid- and far-infrared spectroscopy of galaxies has become possible for sizeable samples with the advent of the Infrared Space Observatory ISO. This paper discusses diagnostics based on emission lines and the mid-infrared emission and absorption features, and their application to starburst galaxies, AGN, and ultraluminous infrared galaxies. The improved understanding of infrared galaxies that has been gained on the basis of the ISO data is of particular relevance for the understanding of the recently discovered infrared galaxies at high redshift. (C) 2002 COSPAR. Published by Elsevier Science Ltd. All rights reserved.
引用
收藏
页码：1989 / 1999
页数：11
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