The infrared morphology of galactic centers

Details The infrared morphology of galactic centers The infrared morphology of galactic centers

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987nascp2466..497t&link_type=abstract

Star formation in galaxies, Proceedings of a conference at the California Institute of Technology, Pasadena, California, June 16

Computer Science

8

Galactic Nuclei, Galactic Structure, Infrared Radiation, Radiation Distribution, Star Formation, Bolometers, Radio Emission, Spatial Distribution, Stellar Spectra

Scientific paper

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.

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