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- W2052475918 startingPage "L77" @default.
- W2052475918 abstract "We report on observations of interstellar dust emission at |b| ≤ 3.°5 and l ∼ 46° with the Far Infrared Photometer (FIRP) on board the Infrared Telescope in Space (IRTS). The FIRP is a four-channel photometer with bands centered at 150, 250, 400, and 700 μm and with a spatial resolution of 0.°5 (FWHM). The 150–250 μm and the 250–400 μm brightness ratios of the interstellar dust emission show a slight decrease with increasing galactic latitude at |b| ≤ 3.°5, consistent with the 140–240 μm brightness ratio observed by COBE/DIRBE. The 250–700 μm brightness ratio shows a much stronger dependence on the galactic latitude. The effect may be due to a single component of warm (T ∼ 20 K) dust with an emissivity index of n < 2, that decreases with galactic latitude. Alternatively, the effect may be due to the existence of two components of dust, a warm (T ∼ 20 K) component and a cold (T ∼ 4–7 K) component, each with an emissivity index of n = 2. In the latter case, either the temperature or the optical depth of the cold component increases as a function of the galactic latitude. In either case, the physical properties of the interstellar dust must be assumed to vary significantly over the range |b| ≤ 3.°5." @default.
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- W2052475918 date "1996-10-01" @default.
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- W2052475918 title "Submillimeter Observations of the Galactic Plane by IRTS" @default.
- W2052475918 doi "https://doi.org/10.1093/pasj/48.5.l77" @default.
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