The stellar populations of dE galaxies in nearby groups

被引:5
作者
Da Costa, GS [1 ]
机构
[1] Australian Natl Univ, Res Sch Astron & Astrophys, Mt Stromlo & Siding Spring Observ, Weston, ACT 2611, Australia
来源
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA | 2004年 / 21卷 / 04期
基金
澳大利亚研究理事会; 美国国家科学基金会; 美国国家航空航天局;
关键词
galaxies : dwarf; galaxies : evolution; galaxies : stellar content; stars : Population II;
D O I
10.1071/AS04044
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this contribution Gemini-North NIRI J, K-observations are used to investigate the upper-Asymptotic Giant Branch (AGB) intermediate-age population in the M81 Group dwarf elliptical (dE) F8D1. Hubble Space Telescope (HST) 'snapshot' V, I-observations are also analysed to investigate the upper-AGB populations in two other M81 Group dEs, DDO 71 and kk077. In all three dEs, significant intermediate-age populations are found. Further, there are sizeable dE-to-dE differences in these populations: F8D1 contains relatively more, and relatively more luminous, upper-AGB stars. These results are compared with existing information for Local Group and Sculptor group dwarfs. It is suggested that 'environmental harrassment' plays an important role in governing dwarf galaxy evolution.
引用
收藏
页码:366 / 370
页数:5
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