Correlation of infrared dust emission, galaxy counts, and hydrogen column density

Details Correlation of infrared dust emission, galaxy counts, and hydrogen column density Correlation of infrared dust emission, galaxy counts, and hydrogen column density

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...289..609d&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 289, Feb. 15, 1985, p. 609-612. Research supported by the Consiglio Naziona

Astronomy and Astrophysics

Astrophysics

8

Cosmic Dust, Far Infrared Radiation, Galaxies, Gas Density, Interstellar Matter, Spatial Distribution, Hydrogen, Optical Thickness

Scientific paper

The authors analyze the correlations of far-infrared emission of
interstellar dust, galaxy counts, and 21 cm atomic hydrogen emission.
They conclude that the IR signal is the best available dust indicator.
The correlations also provide infomation on the inhomogeneity of the
galaxy distribution and on the molecular hydrogen column density.

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