WHAT COBE MIGHT SEE - THE FAR-INFRARED COSMOLOGICAL BACKGROUND

被引：35

作者：

BEICHMAN, CA ^{[1
]}

HELOU, G ^{[1
]}

机构：

[1] INST ADV STUDY,PRINCETON,NJ 08540

来源：

ASTROPHYSICAL JOURNAL | 1991年 / 370卷 / 01期

关键词：

COSMIC BACKGROUND RADIATION; COSMOLOGY; GALAXIES; GENERAL; INFRARED; SOURCES;

D O I：

10.1086/185963

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The redshifted emission from infrared luminous galaxies should produce a diffuse background around 300-mu-m detectable by the Cosmic Background Explorer (COBE). The detection of such emission would provide evidence for evolution in the density or luminosity of galaxies in the infrared.

引用

页码：L1 / L4

页数：4

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