A triple nucleus in the brightest cluster galaxy in Abell 193

被引：9
|
作者：
Seigar, MS
Lynam, PD
Chorney, NE
机构：
[1] Joint Astron Ctr, Hilo, HI 96720 USA
[2] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany
[3] Univ Victoria, Dept Phys & Astron, Victoria, BC V8W 3P6, Canada
来源：
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2003年 / 344卷 / 01期
关键词：
galaxies : clusters : general; galaxies : elliptical and lenticular; cD; galaxies : fundamental parameters; galaxies : individual : IC 1695; galaxies : nuclei; galaxies : structure;
D O I：
10.1046/j.1365-8711.2003.06811.x
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present a ground-based, near-infrared, K-band image and a Hubble Space Telescope (HST) WFPC2 image of the brightest cluster galaxy in Abell 193 (IC 1695). This object was selected as the central cluster galaxy using X-ray information. Both images reveal a triple nucleus structure. Previously, this galaxy was thought to have only two nuclei. We present colours and magnitudes and a colour plot of the three nuclei. The nuclear structure and colours of the nuclei in this galaxy suggest that a merger may have taken place in its recent history.
引用
收藏
页码：110 / 114
页数：5
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