Metallicity gradients in dwarf elliptical galaxies

被引:0
作者
Koleva, Mina [1 ,2 ,3 ,4 ,5 ]
Prugniel, Philippe [3 ,4 ,5 ]
De Rijcke, Sven [6 ]
Zeilinger, Werner W. [7 ]
机构
[1] Inst Astrofis Canarias, E-38200 Tenerife, Spain
[2] Univ La Laguna, Dept Astrofis, E-38205 Tenerife, Spain
[3] Univ Lyon 1, F-69622 Villeurbanne, France
[4] Observ Lyon, CRAL, F-69561 St Genis Laval, France
[5] CNRS, UMR 5574, Paris, France
[6] Univ Ghent, Sterrenkundig Observ, B-9000 Ghent, Belgium
[7] Univ Wien, Inst Astron, A-1180 Vienna, Austria
来源
STELLAR POPULATIONS: PLANNING FOR THE NEXT DECADE | 2010年 / 262期
关键词
galaxies: dwarf; galaxies: elliptical and lenticular; cD; galaxies: stellar content; EVOLUTION;
D O I
10.1017/S1743921310003248
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We discuss the relations between the metallicity gradients and the other characteristics of a set of dwarf elliptical galaxies in different environments dagger. We suggest that dEs have typically metallicity gradients of -0.30 +/- 0.25 dex/r(e), unrelated to their mass. Dwarf elliptical galaxies with embedded disks, or dS0, may have flat metallicity gradients.
引用
收藏
页码:364 / +
页数:2
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