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- W2027330287 abstract "The predicted emission spectrum of galactic dust at about 10 K is compared with the spectrum of 2.8-K universal blackbody radiation and with the spectrum of the anisotropy expected in the 2.8-K radiation due to motion of earth with respect to the coordinate system in which the radiation was last scattered. The extremely anisotropic galactic-dust emission spectrum may contribute a significant background to anisotropy measurements which scan through the galactic plane. The contamination would appear in an 8-mm scan around the celestial equator, for example, as a spurious 200 km/s velocity toward declination 0 deg, right ascension 19 hr, if predictions are correct. The predicted spectrum of dust emission in the galactic plane at longitudes not exceeding about 30 deg falls below the total 2.8-K cosmic background intensity at wavelengths of at least 1 mm." @default.
- W2027330287 created "2016-06-24" @default.
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- W2027330287 date "1977-02-01" @default.
- W2027330287 modified "2023-09-27" @default.
- W2027330287 title "Translational anisotropy in the cosmic microwave background radiation and far-infrared emission by galactic dust clouds" @default.
- W2027330287 doi "https://doi.org/10.1086/182361" @default.
- W2027330287 hasPublicationYear "1977" @default.
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