COSMIC BACKGROUND-RADIATION ANISOTROPIES FROM COSMIC STRUCTURES - MODELS BASED ON THE TOLMAN SOLUTION

被引：50

作者：

PANEK, M

机构：

[1] Copernicus Astronomical Center, 00-716 Warsaw

来源：

ASTROPHYSICAL JOURNAL | 1992年 / 388卷 / 02期

关键词：

COSMIC MICROWAVE BACKGROUND; COSMOLOGY THEORY; GALAXIES CLUSTERING;

D O I：

10.1086/171146

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We investigate anisotropies of the Cosmic Background Radiation (CBR) resulting from second-order gravitational effects in structures like voids, the Great Attractor, and clusters of galaxies. Spherically symmetric models of the structures are based on the Tolman solution of Einstein equations. Predicted anisotropies of the order of 10(-7)-10(-6) are below the sensitivity of present observations.

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页码：225 / 233

页数：9

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