STRUCTURE OF THE GLOBULAR-CLUSTERS IN THE FORNAX DWARF ELLIPTIC GALAXY

被引:18
作者
RODGERS, AW
ROBERTS, WH
机构
[1] Mt. Stromlo Siding Spring O., Institute of Advanced Studies, Australian National University, Weston Creek Post Office, ACT 2611, Private Bag
关键词
D O I
10.1086/116982
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have measured the radial light profiles of the five brighter clusters in the Fornax dwarf elliptical galaxy. We find that the clusters fall into two structural groups. Hodge clusters Nos. 1 and 2 have similar core radii which are twice the core radii of clusters Nos. 3, 4, and 5. Clusters Nos. 1 and 2 appear to fit truncated King models. Clusters Nos. 3, 4, and 5 do not fit the King models but show an extended halo structure with no evidence of tidal truncation. We conjecture that clusters Nos. 1 and 2 have interacted dynamically with each other while the other clusters have had no such interaction over their lifetime.
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页码:1737 / 1744
页数:8
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[31]  
Zinnecker H., 1988, HARLOW SHAPLEY S GLO, P603