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- W202068554 abstract "We review the present understanding of the interstellar dust contribution to the far-IR (λ > 100 μ m) sky emission. We show how the contribution from the distinct ISM components (HI, H 2 , HII gas) are identified and characterized through spatial correlation with gas emission lines. We discuss the spectral energy distribution of the emission from cirrus dust associated with diffuse HI gas and from colder dust associated with molecular gas. We relate the drop in dust emission temperature from the diffuse interstellar medium to molecular gas to an evolution of dust affecting both the abundance of small dust grains and the far-IR emissivity of large grains." @default.
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- W202068554 date "2001-01-01" @default.
- W202068554 modified "2023-09-26" @default.
- W202068554 title "Galactic Far-Infrared Diffuse Emission" @default.
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- W202068554 doi "https://doi.org/10.1017/s0074180900225874" @default.
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