Temperature distribution of interstellar dust

Details Temperature distribution of interstellar dust Temperature distribution of interstellar dust

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...157..393p&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 157, no. 2, March 1986, p. 393-399.

Astronomy and Astrophysics

Astrophysics

58

Cosmic Dust, Interstellar Matter, Temperature Distribution, Absorptivity, Emission Spectra, Energy Distribution

Scientific paper

Using the infrared spectrum (2 μm to 1 mm) of three luminous galactic regions and the absorption properties of interstellar dust, the authors derive its temperature distribution. They also compute the energy output of interstellar dust as a function of temperature. These distributions are bimodal and do not agree with predictions based on standard models, the amount of high temperature dust being much too large.

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