The mid-IR view of interacting galaxies

被引：18
|
作者：
Charmandaris, V [1 ]
Laurent, O
Mirabel, IF
Gallais, P
Sauvage, M
Vigroux, L
Cesarsky, C
Tran, D
机构：
[1] Observ Paris, DEMIRM, Paris, France
[2] Max Planck Inst Extraterr Phys, D-37075 Garching, Germany
来源：
ASTROPHYSICS AND SPACE SCIENCE | 1999年 / 266卷 / 1-2期
关键词：
galaxy; mid-infrared; starburst;
D O I：
10.1023/A:1002693413572
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
In this paper, we present ISOCAM mid-IR broad band images and spectra of three well known interacting galaxies. These are the prototypical ultraluminous IR galaxy Arp 220, and NGC 6240, which are classified as major mergers resulting from a collision of two disk galaxies of approximately equal mass, and the prime example of collisional ring galaxies, the Cartwheel. Our observations provide a new powerful tool and shed some more light to the properties of the hot dust and star formation in interacting galaxies.
引用
收藏
页码：99 / 104
页数：6
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