The colour-magnitude relation of early-type galaxies in the Hubble Deep Field

被引:54
作者
Kodama, T
Bower, RG
Bell, EF
机构
[1] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England
[2] Univ Durham, Dept Phys, Durham DH1 3LE, England
关键词
galaxies : elliptical and lenticular; cD; galaxies : evolution; galaxies : stellar content;
D O I
10.1046/j.1365-8711.1999.02542.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the rest-frame colour-magnitude diagram for 35 early-type galaxies in the Hubble Deep Field with median redshift 0.9. Although they have considerable scatter, a red sequence that is well described by the passive evolution of an intrinsically old stellar population is observed. Comparison with the passively evolved colour-magnitude relation of the rich Coma cluster (z = 0.023) indicates that at least similar to 1/2 of the early-type galaxies in the field at this redshift are as old as those in rich clusters.
引用
收藏
页码:561 / 566
页数:6
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