Globular clusters at low and high redshift

被引：0

作者：

Burgarella, D ^{[1
]}

Chapelon, S ^{[1
]}

Buat, V ^{[1
]}

机构：

[1] CNRS, Astron Spatiale Lab, F-13012 Marseille, France

来源：

ULTRAVIOLET UNIVERSE AT LOW AND HIGH REDSHIFT: PROBING THE PROGRESS OF GALAXY EVOLUTION | 1997年 / 408卷

关键词：

D O I：

暂无

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

Globular clusters can be considered as fossils of the formation of galaxies. Unfortunately, from their present characteristics it seems difficult to extract information on how they formed. We should take advantage of the original burst of globular cluster formation to directly observe newly-born galaxies at UV rest-frame wavelengths (i.e. redshifted in the NIR). This would shed some light on the formation of the parent galaxies.

引用

页码：418 / 422

页数：5

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