CONSTRAINTS ON THEORIES OF GALAXY FORMATION FROM MEASUREMENTS OF FLUCTUATIONS IN THE CMB

被引：2

作者：

REBOLO, R ^{[1
]}

WATSON, R ^{[1
]}

BECKMAN, JE ^{[1
]}

机构：

[1] UNIV MANCHESTER,JODRELL BANK,MANCHESTER M13 9PL,LANCS,ENGLAND

来源：

ASTROPHYSICS AND SPACE SCIENCE | 1989年 / 157卷 / 1-2期

关键词：

D O I：

10.1007/BF00637349

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：333 / 337

页数：5

共 9 条

[1]

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[3]

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[4]

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[5] N-BODY SIMULATIONS OF GALAXY CLUSTERING .3. THE COVARIANCE FUNCTION [J].

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[6] LAMBDA-6-CM OBSERVATIONS OF FLUCTUATIONS IN THE 3K COSMIC MICROWAVE BACKGROUND [J].

LASENBY, AN ;

DAVIES, RD .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1983, 203 (03) :1137-1169

[7]

READHEAD, 1988, PREPRINT

[8] IMPROVED LIMITS ON SMALL-SCALE ANISOTROPY IN COSMIC MICROWAVE BACKGROUND [J].

USON, JM ;

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[9]

WATSON RA, 1988, IAU S

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