Titlebook: Large Scale Structure and Motions in the Universe; Proceeding of an Int M. Mezzetti,G. Giuricin,M. Ramella Conference proceedings 1989 Kluw

stressors

ELUC

向下五度才偏

中子

unstable-angina

sed-rate

The Imprint of Large Scale Structure on the Cosmic Background Radiationrly epochs. This paper reviews recent observational programs to detect such anisotropies on angular scales from 12″ to 8°. That range in angle corresponds to a scale of density perturbations ranging from roughly a galactic mass to more than a supercluster mass. In two cases, there is very tentative

Venules

Peculiar Velocity and Gravity as Cosmological Probesactor infall model and (2) velocity correlation tensor, derived directly from the “.”. Our tests have varying power to constrain theories for the growth of cosmic structure. Each of these tests has its own drawbacks and technical limitations. However, one result seems to be particularly robust: the

chance

猛擊

Baffle