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    The infrared morphology of galactic centers (1987)
    In:  CASI
    Details
    Publication Date: 2013-08-31
    Description: Initial results are presented of a program to map the centers of galaxies in the mid-infrared using the NASA-MSFC 20 pixel bolometer array. Maps at 10.8 micrometer of the galaxies NGC 5236 (M82), NGC 1808, NGC 4536, and NGC 4527 reveal complex emitting regions ranging in size from 500 pc to 2 kpc. The infrared spatial distributions generally resemble those in the visible and radio. In all cases a large fraction of the IRAS 12 micrometer flux originates in spatial structures prominent in the maps.
    Keywords: ASTRONOMY
    Type: NASA, Washington Star Formation in Galaxies; p 497-500
    Format: application/pdf
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