Galaxies and far-infrared emission

Details Galaxies and far-infrared emission Galaxies and far-infrared emission

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...235..392t&link_type=abstract

Astrophysical Journal, Part 1, vol. 235, Jan. 15, 1980, p. 392-404. NASA-supported research.

Other

344

Emission Spectra, Far Infrared Radiation, Galactic Nuclei, Photometry, Broadband, Dust, Galactic Evolution, Interstellar Gas, Milky Way Galaxy, Thermal Radiation

Scientific paper

The far-infrared luminosities of the central few hundred parsecs of many galaxies may exceed by more than an order of magnitude the amount expected from late-type stars. However, for the M82, NGC 253, NGC 1068 and several other galaxies studied in the present paper, the inferred mass-to-luminosity ratios are within the limits expected for stellar distributions containing early-type stars.

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