Galactic dust correlation evidenced by COBE-FIRAS data.

Physics

Scientific paper

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Interstellar Dust: Continuum Radiation

Scientific paper

The authors consider the "warm" and the "cold" components of the galactic continuum dust emission in the COBE-FIRAS high frequency spectra. The spectral models used for these components are two modified blackbodies with ν2 emissivity laws. Using a best-fitting procedure they have obtained two temperature maps and two optical depth maps of the galactic dust emission. The results show that the cold and warm galactic components are well correlated, which support the hypothesis that the cold component may be an unusual spectral feature of dust that gives rise to the warm component.

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