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- W1973212546 abstract "The microwave background radiation is a remnant of the early Universe. It is blackbody radiation with a temperature TCBR = 2.735 ± 0.060 (0.017) K and no measured spectral distortions. It is isotropic to (ΔT/T) < 5 × 10−5 over all angular scales, except for a dipole component which is attributed to our motion with respect to the preferred reference frame of the radiation. A small-scale anisotropy has been detected towards a few dense clusters of galaxies that is attributed to inverse-Compton scattering of the photons of the background radiation by the hot gas that is responsible for the X-ray emission from these clusters. This is the Sunyaev-Zel'dovich effect." @default.
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- W1973212546 date "1992-07-01" @default.
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- W1973212546 title "The microwave background radiation" @default.
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- W1973212546 doi "https://doi.org/10.1016/0920-5632(92)90144-h" @default.
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