A rocket-bornbe measurement of interstellar dust emission at high galactic latitude.

Physics

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Interstellar Dust: Sub-Mm Observations

Scientific paper

The authors have measured the diffuse brightness of the sky in six submillimeter passbands, using a rocket-borne, liquid helium-cooled absolute radiometer. Spatial structure was observed in three shorter wavelength bands, as would be expected for emission from the interstellar dust. The authors have calculated the average column density of H I in each field-of-view along the scan path, using the Bell Laboratories 21 cm survey. The correlation of submillimeter emission with H I column density is shown.

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