Galaxy formation in the IR/submm wavelength range

被引:0
|
作者
Guiderdoni, B [1 ]
机构
[1] CNRS, Inst Astrophys, F-75014 Paris, France
来源
XVTH IAP MEETING DYNAMICS OF GALAXIES: FROM THE EARLY UNIVERSE TO THE PRESENT | 2000年 / 197卷
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中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The ultraluminous IR galaxies unveiled by deep submm surveys very likely are high-redshift merging and interacting systems. The analysis of these observations should provide us with interesting constraints on the evolution of the merging rate in the universe. We briefly review the modelling of ULIRGs in the context of hierarchical galaxy formation and we underline the difficulties.
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页码:421 / 424
页数:4
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