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- W202852017 abstract "Microwave background astronomy has arrived. Largely because of improvements in receivers, the last three years have seen the emergence of agreement concerning important measurements of the microwave background radiation (MBR): – hard evidence that the MBR has a black-body spectrum (see Smoot in these proceedings); – the unambiguous detection of the Sunyaev-Zeldovich decrement in clusters of galaxies (Birkinshaw et al 1984), and indeed profiles of the decrement across clusters (Birkinshaw in these proceedings); – the lack of anisotropy in the MBR temperature T on scales of a few arcmin down to ΔT/T˜5×10 -5 (Uson & Wilkinson 1984; Readhead, private communication) and the consequent elimination of simple theories of adiabatic primordial fluctuations." @default.
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- W202852017 date "1986-01-01" @default.
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- W202852017 title "The Microwave Background from Cambridge" @default.
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- W202852017 doi "https://doi.org/10.1017/s1539299600006596" @default.
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