ISO spectroscopy of luminous infrared galaxies

被引：0
|
作者：
Genzel, R [1 ]
Lutz, D [1 ]
机构：
[1] Max Planck Inst Extraterr Phys, D-85740 Garching, Germany
来源：
SPACE INFRARED TELESCOPES AND RELATED SCIENCE | 2000年 / 25卷 / 11期
基金：
美国国家航空航天局;
关键词：
D O I：
10.1016/S0273-1177(99)01160-6
中图分类号：
V [航空、航天];
学科分类号：
08 ; 0825 ;
摘要：
Spectroscopy from the Infrared Space Observatory ISO has for the first time provided the sensitivity to observe mid-infrared fine structure lines and PAH features in a wide range of luminous infrared galaxies. We report on observations obtained with SWS, ISOPHOT-S, and the ISOCAM CVF and show that the mid-IR spectral features are excellent diagnostic tools to distinguish starburst from active galactic nuclei activity and analyze their properties. We find that the majority of the most luminous infrared galaxies are likely predominantly powered by star formation. (C) 2000 COSPAR. Published by Elsevier Science Ltd.
引用
收藏
页码：2243 / 2249
页数：7
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