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- W2034893438 abstract "A test is proposed of the hypothesis that the large-scale distribution of galaxies is generated by large-scale pressure gradients in protogalactic gas, due to pregalactic explosions or other inhomogeneous energy sources at redshifts z< or approx. =10. Pressure inhomogeneities in hot gas lead to anisotropy in the microwae background via the Sunyaev-Zel'dovich Compton heating effect. The amplitude of the predicted anisotropy is estimated using simplified models is found to conflict with current upper limits. Several possible complications are considered and are found to increase the predicted anisotropy. Hydrodynamical effects may significantly affect the matter distribution on galactic scales but probably cannot produce the large-scale galaxy clustering on scales of the order of approx.10 Mpc without violating this constraint." @default.
- W2034893438 created "2016-06-24" @default.
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- W2034893438 date "1984-09-01" @default.
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- W2034893438 title "Microwave background anisotropy and hydrodynamic formation of large-scale structure" @default.
- W2034893438 doi "https://doi.org/10.1086/184339" @default.
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